The galaxy presents as a centrally concentrated, elliptical-like structure with a relatively smooth appearance. A dominant, bright core region is evident, suggesting a high stellar density. The overall shape appears elongated, approaching a cigar-like form. There's a noticeable gradient in brightness, decreasing from the core outwards. Some subtle hints of faint, diffuse outer regions are visible, although the lack of defined spiral arms or prominent features indicates a relatively quiescent morphology. No obvious signs of major mergers or significant tidal disturbances are apparent in the immediate vicinity. The color profile suggests a relatively older stellar population, exhibiting a yellowish hue in the central regions, potentially indicating a reduced rate of ongoing star formation, though there may be some star formation occurring.
