The galaxy presents as a smooth, centrally concentrated object with a roughly elliptical morphology. Its core is bright and exhibits a yellowish hue, indicating a population of older stars. A gradual decrease in luminosity extends outwards from the core. The overall color profile suggests relatively low levels of ongoing star formation and a dominance of older stellar populations. There is no apparent spiral structure or bar feature. Minor irregularities appear in the outer regions which may be tidal debris or small disturbances.
