The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that appears yellowish in color, suggestive of an older stellar population. The light distribution appears diffuse, without prominent spiral arms or distinct features, indicating a lack of significant ongoing star formation. The galaxy appears moderately elongated, showing that it is not perfectly spherical. There is no indication of any major merging events, and the system appears relatively isolated. 
