The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that appears roughly circular in projection. The light profile appears to gradually decrease from the center outwards, lacking sharp edges or prominent spiral arm structures. 

Color gradients are subtle, with a central region appearing more yellow, suggestive of an older stellar population with relatively little ongoing star formation. The outer regions may be slightly redder, though the faintness of these areas makes precise color determination difficult.

There is no obvious evidence of a recent major merger or tidal interactions, with minimal visible disturbance to the galaxy's overall structure. The galaxy appears relatively isolated and undisturbed.
