The observed galaxy presents a generally elliptical morphology, appearing somewhat flattened along its major axis. A bright, concentrated central bulge is evident, displaying a yellowish-white color, indicating an older stellar population. The surrounding halo exhibits a more diffuse, fainter luminosity, with a subtle gradient towards the outer edges. Hints of dust lanes or patchy structures are possibly present within the halo, potentially suggesting interactions or ongoing accretion events. The galaxy's overall color appears slightly redder than average, which would be consistent with a later-type stellar population. A slight asymmetry in the outer regions may suggest the presence of a minor tidal disturbance or past merger event, although the structure appears mostly relaxed.
