The galaxy presents as a generally smooth, elliptical-like structure with a concentrated central bulge. The light distribution is highly concentrated towards the center, exhibiting a radial falloff in intensity. The color profile indicates a population of older stars, seen through the yellow-red hue of the galaxy. There is no evidence of active star formation regions, spiral arms, or strong dust lanes from the image. The shape appears mostly round, without significant elongation or distortion. Faint, diffuse light extends outward from the core but remains mostly amorphous and without distinct features. It does not appear to be interacting with other galaxies, showing no signs of tidal tails or disrupted morphology.
