The galaxy presents as a relatively smooth, centrally concentrated object, elliptical in shape, with a major axis appearing slightly longer than its minor axis. The light profile shows a bright, compact core that diffuses outwards to a fainter halo. The color distribution is not uniform across the galaxy. The core presents a more yellow-orange hue, which may indicate a population of older stars. Moving towards the outer regions of the galaxy, there is a subtle shift toward bluer colors, possibly from a younger stellar population or on-going star formation, albeit at a low rate. There are hints of minor disturbances in the outer halo, which could be tidal streams or debris from past interactions, though the main structure appears largely undisturbed.
