The galaxy presents a generally smooth morphology with a slightly elongated, ellipsoidal shape. The central region exhibits a bright, concentrated bulge, characterized by a yellowish-orange hue. The overall color profile suggests a population of older stars dominating the core. Moving outwards from the center, a faint, diffuse disk component can be discerned. Hints of bluer regions are visible within the disk, possibly indicative of ongoing or recent star formation. The disk is not particularly well-defined, lacking prominent spiral arm structures. There appears to be a minor disturbance or tidal feature potentially indicative of a past or ongoing interaction with another galaxy.
