The galaxy presents a somewhat elliptical morphology, appearing as a flattened spheroid. Its light profile suggests a relatively smooth distribution, with a gradual decrease in intensity from the central region outwards. There is a subtle indication of a possible disk-like structure, though it is not sharply defined. The galaxy exhibits a predominantly blue hue, indicative of a population of young, hot stars and ongoing star formation. There is a slight suggestion of asymmetry within the galactic structure, possibly indicating minor gravitational disturbances or interactions. No major tidal features are evident. The galaxy appears relatively isolated, showing no signs of a major merger event in its recent past.
