The galaxy presents an elongated, cigar-shaped morphology. It exhibits a smooth, featureless appearance in the optical bands, lacking prominent spiral arms or distinct dust lanes. The galaxy's light profile suggests a concentration of older stellar populations. The core region is slightly brighter than the outer regions. The color gradient is subtle, transitioning from a yellowish center to a slightly bluer, fainter periphery, suggesting possible on-going, but low, star formation. The galaxy appears relatively undisturbed, lacking any strong tidal features or indications of a major merger. There may be evidence of a minor disturbance, visible as a slight asymmetry.
