The galaxy presents as a relatively smooth, elliptical-like structure. The light distribution appears centrally concentrated with a bright core region, suggesting a high stellar density in the nucleus. There is little evidence of distinct spiral arm structures or prominent dust lanes. The galaxy exhibits a generally rounded morphology. A subtle color gradient is observed, with a slight bluer tint around the outer edges of the galaxy in contrast to the inner core of the galaxy. There is no obvious presence of major merging activity, though there may be some minor disturbances.
