The galaxy presents as an elliptical structure with a relatively smooth light distribution. The central region is brighter, with the overall shape appearing close to round. There is some evidence of a possible minor disturbance or interaction, given the slightly irregular shape and light distribution. The color profile indicates a mix of stellar populations. The central region appears to have a bluer hue, suggesting the presence of younger stars or ongoing star formation. The outer regions exhibit a reddish tint, consistent with an older stellar population.
