The galaxy presents as an elongated, somewhat spindle-shaped structure, appearing significantly longer than it is wide. The overall color is a blend of pale yellow and white, suggestive of an older stellar population with fewer active star-forming regions. There may be a slight hint of bluish colors at the edges, which could indicate the presence of some younger, hotter stars, but this is not as prominent.

The galaxy appears largely smooth in texture. There are no obvious spiral arms or other distinct features. Its central region exhibits a brighter and more concentrated luminosity, likely indicative of a dense stellar nucleus or bulge. There's no evidence of significant dust lanes or other obscuring material, which allows a clear view of the galaxy's primary structure.

There seems to be minimal ongoing star formation, the overall color and smooth morphology are consistent with an early-type galaxy, possibly an elliptical or lenticular galaxy viewed edge-on. This galaxy is likely a mature system where star formation has largely ceased, resulting in an older and redder stellar population. There are no signs of major disturbances or interactions with other galaxies.
