The galaxy presents as a largely featureless elliptical object. It exhibits a high degree of central concentration with a relatively smooth luminosity profile, suggesting a population dominated by older stars. The galaxy appears largely spheroidal. There is evidence of minor tidal disturbances or interactions, potentially indicating a recent merger event. While the overall color appears to be yellowish, there are hints of bluer regions, which may correspond to areas of ongoing or recent star formation, though at a low rate. The galaxy's apparent magnitude suggests a substantial luminosity.
