The galaxy presents a generally smooth morphology with a dominant, rounded structure. Its color profile suggests a population of older stars, biased towards the redder end of the spectrum, possibly due to a lower rate of recent star formation. There is a subtle hint of a disk-like structure, but this is not well-defined, and the galaxy appears primarily spheroidal. No strong tidal features or other indications of recent major merger events are apparent, though minor disturbances cannot be ruled out. The galaxy appears relatively isolated.