The galaxy exhibits an elliptical morphology, appearing generally smooth and centrally concentrated. A slight elongation is apparent, with the major axis extending in a roughly horizontal direction. The central region displays a bright, yellowish hue, indicative of an older stellar population and potentially a significant bulge component. Moving outwards, the light gradually fades, exhibiting a transition to redder tones, and the outer regions blend subtly into the background sky. There is no clear evidence of spiral arm structures or prominent dust lanes. The galaxy appears relatively undisturbed, showing no strong signs of recent major mergers or tidal interactions. The overall color suggests a passively evolving system with a suppressed star formation rate.
