The galaxy appears as a single, relatively smooth object, with a dominant central bulge. The light profile suggests a concentrated core. The galaxy exhibits an elliptical shape, tending towards roundness, with minimal indication of spiral arm structures or a prominent disk. There seems to be a tidal tail or an object it could be interacting with, based on its apparent location, size, and color.

The galaxy exhibits a color gradient, with a redder core transitioning to bluer outer regions. The central region appears yellowish-orange, possibly indicative of an older stellar population or dust obscuration. The faint, bluer regions on the edges suggest the possibility of ongoing, though perhaps limited, star formation within this galaxy. There does not appear to be any significant dust lane or patchiness in the light distribution.
