The galaxy presents a somewhat diffuse morphology, with an overall elliptical shape. The light distribution appears relatively smooth, suggesting a lack of prominent spiral arms. A slightly brighter, more concentrated central region or nucleus is observed. There is a suggestion of some distortion in the galaxy's overall shape, and possible evidence for a minor disturbance. There may be some ongoing or recent merger activity, or interaction with a smaller companion galaxy.

Color gradients across the galaxy are subtle, but a slightly bluer tint is observed in the outer regions, possibly indicative of younger stellar populations or ongoing star formation, with the inner region appearing more yellow. The galaxy is relatively compact in size.
