The galaxy exhibits a generally elliptical morphology, appearing somewhat elongated with an axial ratio of approximately 0.7. The light distribution is centrally concentrated, displaying a smooth and gradual decline in surface brightness outwards from the core. There is little to no evidence of distinct spiral arm structure or prominent dust lanes visible. The overall color appears to be relatively uniform and reddish, suggestive of an older stellar population and potentially reduced ongoing star formation. The light is fairly uniform across the galaxy, with only minor colour variations. There are no signs of any major disturbances to the galaxy from other objects or ongoing mergers.
