The galaxy presents as a singular, centrally concentrated object. It exhibits a generally smooth morphology, with no apparent spiral arms or a distinct disk structure visible in this image. The galaxy appears largely elliptical in shape, though there is some deviation from perfect circularity. The light profile suggests a concentrated central bulge with a relatively gradual decrease in luminosity moving outward. The central region is notably brighter and appears to be more yellowish in color compared to the outer regions, suggesting a population of older stars. There's some evidence of bluer light in the outer regions, potentially indicative of ongoing star formation, albeit at a low level. There is no strong evidence of any major mergers or tidal disturbances. A minor asymmetry or irregularity is not ruled out.
