The galaxy presents as a relatively smooth, elliptical-like structure with a highly concentrated central bulge. The light distribution appears centrally concentrated, with a gradual decrease in intensity outwards from the core. There is little indication of distinct spiral arm structures or prominent dust lanes. The galaxy exhibits a slight elongation, suggesting a classification somewhere between round and cigar-shaped. The color profile seems relatively uniform across the visible spectrum with possibly more blue in the center, indicating moderate amounts of ongoing star formation. No signs of major mergers or significant tidal disturbances are apparent within the immediate vicinity of the galaxy.
