The galaxy presents as a relatively smooth, centrally concentrated object. Its overall form appears mostly round, with a slight suggestion of elongation. The light profile suggests a dominant spheroid component. There appears to be little or no evidence of spiral arm structure or a prominent disk.

In terms of color, the galaxy exhibits a broad yellow to orange hue, becoming redder at the periphery. This suggests a stellar population that is dominated by older, cooler stars and relatively low ongoing star formation. The overall color profile is consistent with an elliptical galaxy or a lenticular galaxy seen face-on.

There is no indication of strong tidal features, major disturbances, or ongoing mergers. The surrounding region appears relatively undisturbed, with no obvious companion galaxies interacting with the primary object. The galaxy is moderately bright, suggesting a high intrinsic luminosity. The estimated physical size is approximately 6 kpc in radius.
