The galaxy appears to be a relatively smooth, elliptical galaxy, with a noticeable bulge and a slight elongation. The central region exhibits a bright, concentrated light profile, suggesting a high stellar density within the galactic nucleus. There is a subtle color gradient, shifting from a slightly bluer hue towards the outer edges to a yellower, redder core. The absence of prominent spiral arms or dust lanes indicates a lack of significant ongoing star formation. Slight disturbances in the shape and light distribution suggest minor tidal interactions or past merger events. The overall structure indicates a mature galaxy which is consistent with minimal star formation.
