The galaxy presents a somewhat irregular morphology. It appears to be undergoing a possible interaction or disturbance, indicated by a slight elongation or tidal feature extending from its main body. The central region of the galaxy exhibits a concentrated luminosity, suggesting the presence of a bulge or active galactic nucleus. The overall color is indicative of an older stellar population. Evident of a substantial mass, with indications of active, though not extreme, star formation. It may be classified as an elliptical galaxy.
