The galaxy presents a predominantly smooth morphology. The central region is noticeably bright, with a concentrated luminosity profile suggesting a significant stellar population. The overall shape is elliptical to slightly disk-like, leaning towards a more rounded appearance, with subtle color variations that could indicate differing stellar populations or dust distribution. There is evidence of a minor disturbance or possible interaction, where a faint, diffuse structure is observed, potentially indicating a tidal feature or a less significant merger event. Overall, the galaxy displays a fairly undisturbed and smooth appearance.
