This galaxy presents a generally smooth, elliptical morphology. Its light profile is dominated by a bright, concentrated central region that fades gradually outwards. There is no clear evidence of spiral arms or a distinct disk structure. The galaxy exhibits a slight elongation, deviating marginally from a perfect circle. There is no obvious indication of strong tidal features or ongoing major merger activity, although a faint asymmetry may suggest minor disturbances or interactions in its recent past. The color gradient appears relatively uniform, with a central core showing a yellowish-white hue, indicative of an older stellar population. The overall appearance suggests a mature system with ongoing, but likely low, levels of star formation.
