The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. There's a gradual decrease in luminosity from the core outwards, suggesting a fairly even distribution of stars. The lack of distinct spiral arms or prominent dust lanes indicates a possible classification as an early-type galaxy. The galaxy exhibits a slight elongation, deviating from a perfectly circular shape, hinting at a possible deviation from a perfect sphere and/or the presence of a disk. There is no noticeable sign of on-going merger activity or major disturbances.
