The galaxy presents as a somewhat elongated structure, approximately elliptical in appearance. The central region displays a concentrated, bright core that suggests a high density of stars or an active galactic nucleus. Moving outward from the center, the light gradually diffuses, transitioning into a fainter halo region. The overall color profile appears relatively uniform across the galaxy, with a slight shift towards redder hues, particularly in the outer regions, possibly indicating an older stellar population. Evidence of a disk is possibly present, though not obviously, and the overall structure is relatively smooth with no clear signs of active star formation or spiral arms. Subtle disturbances or irregularities appear in the outer regions of the galaxy which could be indicative of an ongoing or past merger event. The galaxy exhibits a moderate level of elongation, appearing more lenticular than perfectly spherical.
