The galaxy presents an elliptical morphology, appearing largely smooth with a dominant central bulge that emits strongly. The light profile suggests a primarily older stellar population within the bulge, indicated by the reddish-yellow hue. There's a subtle hint of a disk structure, possibly very faint, around the central region. There is a suggestion of a minor disturbance possibly indicative of a minor gravitational interaction event, or perhaps the initial stages of a tidal disruption or a merger with a smaller object.