The galaxy appears to be an elliptical type, exhibiting a centrally concentrated light profile with a smooth, diffuse appearance. The main body of the galaxy is elongated, showing a distinct major and minor axis. The central region is bright, decreasing in luminosity as it reaches its outer edges. The galaxy has a slight tilt relative to our line of sight, appearing flattened. Faint extensions are visible near the poles, which might suggest interactions or past mergers, but could also be attributed to image artifacts or faint tidal features. The color of the galaxy is primarily a muted yellow-white, suggesting a population of older stars and a lack of significant ongoing star formation within the main body. There is a slight hint of bluer light towards the outer edges, potentially indicating the presence of younger stellar populations in the outskirts or some remaining residual star formation.
