The galaxy presents a generally elliptical morphology, with a smooth, diffuse light distribution indicative of an early-type galaxy. The central region is significantly brighter and concentrated, suggesting a prominent galactic nucleus. The galaxy's color appears to be predominantly yellow-orange, which implies an older stellar population with a lower rate of recent star formation. There is minimal evidence of spiral arm structure or dust lanes. The galaxy exhibits an intermediate ellipticity, appearing somewhat flattened rather than perfectly spherical. The outer edges of the galaxy fade gradually into the background, indicating a lack of sharp boundaries or tidal features. There are no signs of ongoing major mergers or significant morphological disturbances, although some subtle asymmetry in the outer halo cannot be entirely ruled out.
