The galaxy presents as a somewhat compact object, exhibiting an elliptical morphology. The light distribution appears relatively smooth, with a central concentration and a gradual decrease in surface brightness towards the outer regions. There is a suggestion of asymmetry, potentially indicating a minor interaction or disturbance. Color gradients are subtle, trending towards redder hues in the central region and a slightly bluer tint in the outer areas, indicative of a possible mix of stellar populations with varying ages. There does not seem to be any sign of a clear spiral arm structure. The scale of the galaxy suggests it is a relatively average-sized galaxy. There are not any signs of strong tidal tails or significant morphological distortions indicative of an ongoing major merger event.
