The galaxy presents as a fairly compact, elliptical-like structure. Its luminosity profile appears smooth and concentrated towards the center, suggesting an older stellar population. The galaxy exhibits a moderate red color, potentially indicative of evolved stars and a lower rate of ongoing star formation. There is no clear evidence of a prominent disk or spiral arms. The isophotes, while not perfectly circular, are more rounded than elongated, placing it as not cigar shaped, but somewhere in-between a circle and cigar shape. There is no obvious indication of major tidal disturbances or ongoing mergers, although slight asymmetry cannot be completely ruled out. The object seems relatively isolated within its immediate field.
