The galaxy presents as a moderately luminous object with a generally smooth and elliptical morphology. Its core region exhibits a concentrated yellowish-white hue, suggesting a population of older stars. Moving outward from the core, a subtle transition to a bluer color is observed, hinting at the presence of a younger stellar population potentially associated with ongoing, albeit subdued, star formation. The galaxy's overall shape appears somewhat elongated. There is a suggestion of minor disturbances in its structure, possibly indicative of past or ongoing interactions with other galaxies, though no major mergers appear to be present.
