The galaxy appears to be of a generally smooth morphology. It exhibits a somewhat regular elliptical shape, though not perfectly round, tending toward a more intermediate elliptical form. A slight central bulge is observed with a concentration of light intensity at the nucleus. No distinct spiral arms are readily apparent; however, subtle features hinting at a disk-like structure may be present but are difficult to resolve given image quality. The galaxy exhibits a color gradient, with the central bulge appearing more yellowish, possibly indicating an older stellar population and a higher concentration of dust. Moving outward from the core, the galaxy's light appears to be somewhat bluer, hinting at younger stars in the galaxy's outer regions. There is no evidence of a strong tidal interaction or ongoing major merger events. Some minor disturbance in shape is slightly visible; however, these are faint. No obvious dust lanes are apparent, and the overall structure suggests an evolved system.
