The galaxy appears as a relatively smooth, elliptical-like structure. There is an indication of a central bulge with the luminosity appearing more intense in the core. The overall shape is somewhat rounded but deviates slightly from perfect circularity. There are no readily apparent spiral arms or significant dust lanes. The galaxy's color profile suggests a higher concentration of older stellar populations. The overall morphology is fairly undisturbed, with minimal evidence of any recent major mergers or tidal interactions. Faint, diffuse extensions may indicate minor disturbances.
