The galaxy presents an elliptical morphology, appearing largely smooth and featureless. The light distribution is centrally concentrated, with a bright core region transitioning to a more diffuse outer halo. The color profile suggests a predominantly older stellar population, evidenced by the reddish hue in the outskirts, with the very inner core showing a slight yellow-green tint. The overall roundness of the galaxy suggests a classification tending away from spiral or highly irregular forms. No distinct spiral arms, bars, or significant tidal disturbances are discernible. The galaxy exhibits a level of uniformity which indicates it is potentially an early-type galaxy, possibly of substantial mass. There is no apparent evidence of ongoing major merger activity, although there is some slight distortion on the outskirts. The estimated size of the galaxy is consistent with that of a large galaxy, spanning multiple kiloparsecs in diameter.
