The galaxy presents as a smooth, elliptical morphology. The central region exhibits a concentrated, bright core, suggestive of an older stellar population. Moving outwards from the core, there is a gradual decrease in luminosity and a slight color gradient. The lack of discernible spiral arms or prominent dust lanes indicates a relatively quiescent state of star formation within the galaxy. The overall shape is somewhat rounded, but with a slight elongation, resembling an oblate spheroid. There is no clear evidence of recent or ongoing major mergers or tidal disturbances affecting its structure.
