The galaxy presents a generally smooth, elliptical morphology. The core region is luminous, exhibiting a yellowish-white hue, suggesting a population of older stars. Faint blue-ish edges may indicate younger stars beginning to form in its periphery. There is no apparent spiral structure or well-defined dust lanes. The round, symmetrical appearance indicates minimal tidal disruption or interaction with other galaxies. The overall color profile suggests an evolved stellar population with some recent star formation activity. There does not appear to be any ongoing merging activity.