The galaxy presents as a moderately luminous elliptical structure. The core exhibits high surface brightness, with a concentrated yellowish emission, indicative of an older stellar population. The object appears somewhat elongated, displaying a cigar-like shape. The outer regions show a gradual decrease in surface brightness, with some subtle hints of disk-like structure. There does not appear to be any ongoing major merging activity or significant tidal disruption. There may be signs of minor disturbances, but these are difficult to confirm with the resolution of the image. The overall color suggests a relatively quiescent star formation rate, consistent with a dominant population of older stars.
