The galaxy presents as an elliptical morphology, with a smooth light distribution suggesting a relatively evolved stellar population. The central region exhibits a higher surface brightness and a yellowish hue, potentially indicative of older, cooler stars. Moving outward, the light gradually decreases in intensity. At one end of the galaxy is an area with a slightly reddish tint, which could suggest some ongoing star formation activity or a dust lane that is reddening the light. There seems to be some tidal disturbances with some minor tail formation on each end. The galaxy is somewhat elongated. The light distribution is generally even, with no strong evidence of spiral arms or distinct features beyond the tidal disturbances.
