The galaxy presents a somewhat elongated, elliptical morphology. There is a central concentration of light, suggesting a bulge. The disk is not clearly defined, but there is a noticeable flattening along the major axis. The galaxy exhibits a smooth appearance with an overall bluish tint, particularly in the outer regions, suggestive of recent or ongoing star formation. There are hints of disturbances in the morphology, possibly indicating an interaction or merger event. There appears to be some asymmetry in the light distribution. The galaxy shows a generally smooth profile, indicative of an evolved stellar population.
