The galaxy exhibits a generally smooth morphology. It appears elliptical in shape, with a moderate elongation along its major axis. The light distribution is concentrated toward the center, suggesting a dominant bulge component. A subtle color gradient is observed, with the central region appearing more yellow, possibly indicative of an older stellar population, while the outer regions show a slight bluer tint, hinting at the presence of younger stars or ongoing star formation activity, however minimal. There is no strong evidence of spiral arms or a well-defined disk structure. No signs of major mergers or significant tidal disturbances are apparent, though a very minor asymmetry cannot be ruled out.
