The galaxy presents as an elliptical morphology, with a cigar-like shape. There is a smooth, centralized concentration of light indicative of an older stellar population dominating the core. Moving outwards, a subtle gradient of blue suggests areas of active, ongoing, but limited star formation within the galaxy's structure. Faint wisps of asymmetry or minor disturbances are present within the galaxy disk, though not indicative of a major ongoing merger event. The overall smooth appearance suggests a system undergoing some interaction, but primarily dominated by well-established morphology.
