The galaxy exhibits a generally elliptical morphology, appearing somewhat flattened. Its luminosity profile suggests a central bulge region that gradually fades into the outer regions. There is little to no evidence of spiral arm structure or significant dust lanes. The color gradient indicates a possible redder core, suggesting an older stellar population concentrated at the center, with bluer, possibly younger stars distributed in the surrounding regions. There might be a very subtle disturbance hinting at a past or ongoing minor interaction, but it's largely a smooth, relatively undisturbed system. The object appears fairly compact, with a moderately high surface brightness.
