The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a bright, concentrated core, likely indicating a high density of stars. There is a gradual decrease in luminosity from the core outwards, with a faint, extended halo enveloping the central structure.  A subtle color gradient is observed, with the core appearing more yellow, potentially suggestive of an older stellar population, while the outer regions show hints of bluer hues. The overall shape is close to round, though there may be some subtle deviations that could indicate tidal interactions or past mergers. There is some visual evidence of minor disturbance in the outer regions of this galaxy, which may be linked to ongoing or past interactions.
