The galaxy presents a generally smooth morphology. It appears to be disk-dominated but moderately disturbed. The primary body of the galaxy exhibits a bulge. The overall shape is elongated, neither perfectly round nor highly flattened, suggestive of a disk galaxy viewed at an intermediate inclination. There's asymmetry in the outer regions, potentially indicating minor tidal disturbances or interactions with nearby objects. The light profile is concentrated toward the core, with a gradual decrease in surface brightness outwards. Some irregularities in the disk are present, but not pronounced enough to classify it as a major merger. Its color suggests a significant population of older stars. Star formation appears suppressed or minimal throughout the disk.
