The galaxy presents as a single, relatively symmetrical, concentrated object. Its light profile appears smooth and largely featureless, suggesting a classification as an elliptical galaxy. A spherical or slightly flattened spheroidal shape seems likely. The color gradient indicates that the central region has a higher concentration of older stars, as evidenced by the yellower hue. The outer regions appear slightly bluer, indicative of some younger stellar populations and/or ongoing star formation, although overall the galaxy appears quite red. There is no visual evidence of spiral arms, bars, or significant dust lanes. The object appears isolated, with no obvious signs of tidal interactions or recent mergers, although there is a relatively high probability of minor disturbance.
