The galaxy presents as a relatively smooth, luminous structure. Its shape appears moderately elliptical, not perfectly spherical but also lacking a highly elongated, cigar-like appearance. There may be a slight hint of a disk-like component or faint arms, or perhaps a tidal disturbance, but such features are not clearly defined. The central region appears brighter and more concentrated than the outer regions, indicative of a central bulge. Evidence suggests it has undergone, or is undergoing, some level of merger or interaction with another galaxy. The overall color suggests a population dominated by older stars, potentially with ongoing low-level star formation.
