The galaxy presents with a roughly elliptical morphology, though some minor irregularities are present. The light distribution suggests a concentration of older stars in the center of the galaxy, with a more diffuse distribution of younger stars visible in the outer regions. The galaxy exhibits a blueish hue in its outer regions, indicative of ongoing star formation. No spiral arm structures are clearly discernible. There are no strong indications of a major ongoing merger, though some tidal debris may exist.
