The galaxy presents as a luminous, elliptical structure. The central region exhibits a high degree of brightness, suggesting a concentrated core. Moving outward, the light gradually diminishes into a diffuse halo. The overall color profile indicates a population of older stars, likely lacking significant recent star formation. The galaxy appears relatively undisturbed, without obvious signs of ongoing mergers or tidal interactions, although some minor disturbances cannot be ruled out. Its shape is elongated, possibly indicative of a flattened spheroidal system, leaning towards a cigar shape.
