The galaxy appears to be an elliptical type, exhibiting a generally smooth and round morphology. The light is concentrated towards the center, with a gradual decrease in intensity outwards. There is a noticeable color gradient, with the central region displaying a yellowish hue, suggesting an older stellar population, while the outer regions appear slightly bluer, possibly indicating the presence of some younger stars, even if at low levels. There is a slight distortion of the overall shape. This may suggest a potential interaction or past merger event with another galaxy, though no other objects are obviously close enough to be causing that event. The lack of obvious spiral arm structure or significant dust lanes further supports its classification as an elliptical galaxy.
