The galaxy presents as a generally smooth, elliptical-like object with a slight elongation. It exhibits a concentrated central bulge that is yellowish in color, suggesting an older stellar population dominating the core. Fainter, bluer regions extending outwards from the central bulge might indicate areas of ongoing star formation. There are no clear spiral arm structures visible; instead, the light appears diffuse and somewhat irregular at the edges. There is evidence of what might be a minor tidal disturbance or interaction with a smaller companion galaxy, resulting in an asymmetrical halo surrounding the main galaxy. A portion of the galaxy appears distorted, suggesting it may be in the early stages of a merger.