The galaxy appears as a diffuse, elongated structure with a relatively smooth overall appearance. Its shape is somewhere between rounded and cigar-shaped. A concentration of light is seen centrally, suggesting the presence of a galactic bulge or core. There is a faint blue tinge along the edges of the galaxy, possibly indicating regions of younger, hotter stars or active star formation. The main body of the galaxy exhibits a yellow-white hue, which could represent an older stellar population. No distinct spiral arms or prominent dust lanes are readily apparent at this resolution, contributing to the galaxy's smooth, featureless character. There are no obvious signs of major disturbances or ongoing mergers.
