The galaxy presents a generally smooth, somewhat rounded morphology. It exhibits a central bulge which appears relatively bright and concentrated. The color profile suggests a mix of stellar populations, with a slight bluer hue concentrated in what may be a faint disk or arm-like features. Evidence suggests some form of interaction, as the morphology shows some disturbance. There appears to be a smaller object that may be associated with the galaxy, hinting at a possible ongoing or past merger event. Although generally smooth in appearance, there is slight unevenness to the brightness.
