The galaxy presents as a predominantly smooth, elliptical-like structure. A concentrated central bulge emits a yellowish hue, potentially indicating an older stellar population. Moving outward from the core, the light gradually diffuses with a more greenish tint. The overall rounded shape suggests a relatively relaxed system, seemingly undisturbed by recent major merger events. There is a slight suggestion of a faint, disk-like structure, though the smooth light profile dominates. The galaxy exhibits a moderate size and luminosity. Star formation appears to be present, albeit at a modest rate, considering the apparent lack of bright, blue star-forming regions.
