The galaxy presents as a largely featureless elliptical or lenticular system. The light profile appears smooth and centrally concentrated with no discernable spiral arm structures, dust lanes, or prominent star-forming regions visually apparent in this observation. There is a suggestion of a slight elongation, potentially indicating a disk component, but the overall shape appears primarily spheroidal. The core is noticeably bright, likely due to a concentration of older stellar populations and possibly a supermassive black hole at its center. The galaxy appears to be relatively isolated with no obvious tidal features or close companion galaxies suggesting recent merger activity. Its color appears relatively uniform and lacks the patchy blue regions indicative of active star formation.
