The galaxy presents as a relatively smooth and concentrated object. Its overall morphology appears to be elliptical, with a bright central bulge region that dominates the light output. The radial light profile decreases steadily outwards from the core, with no obvious spiral arm structures or prominent star-forming regions visible. There is a slight elongation, not quite a perfect sphere, and a hint of asymmetry in the outer regions, potentially suggesting a mild tidal interaction or past merger event. The color appears generally redder, especially within the central regions, implying an older stellar population. Any active star formation is likely suppressed, judging by the lack of blueish regions. Overall, it presents as a fairly passive galaxy.
