The galaxy presents as a single, relatively concentrated object with a smooth, elliptical morphology. The central region exhibits a bright, yellowish-white core, suggesting a dense population of older stars. The intensity of the core decreases gradually outwards. The overall color is on the redder side, consistent with a population of aging stars and relatively low levels of ongoing star formation. There appears to be a slight asymmetry or disturbance in the halo to the south, possibly indicating a minor tidal interaction or past merger event. There is no readily apparent disk structure or spiral arms.
