The galaxy presents as an elongated, cigar-shaped structure. It is likely a spiral galaxy viewed at a high inclination, or potentially an elliptical galaxy with a prolate shape. The central region exhibits a brighter, concentrated core. The color gradient shows a redder hue in the core transitioning to a bluer tint towards the outer regions. Some evidence of a faint disk can be observed. No spiral arms are clearly visible. There might be some interaction or minor disturbance occurring, but the overall structure appears relatively undisturbed.
