The galaxy presents as a luminous elliptical structure, appearing largely smooth with a highly concentrated central bulge. There is a noticeable fall-off in luminosity from the core outward. The galaxy appears more elongated than spherical. The color profile suggests a population dominated by older stars, with a yellowish hue permeating the galaxy's overall appearance. No distinct dust lanes or spiral arm structures are visible. There may be some very faint evidence of a slight disturbance to its morphology, but overall appears to be an isolated system without significant tidal interactions.
