The galaxy presents a largely smooth, elliptical morphology. There is a slight elongation, appearing somewhat football-shaped rather than perfectly spherical. The central region is characterized by a bright, concentrated core, suggesting a high stellar density. The light profile appears to fade gradually from the core outwards, with no distinct spiral arm features or prominent dust lanes visible. The overall color is a yellowish-orange hue, indicative of an older stellar population and low levels of ongoing star formation. There is no indication of significant tidal disturbances or ongoing mergers. The galaxy appears to be relatively isolated within its field of view.
