The galaxy presents an elliptical morphology, with a high degree of central concentration. The core exhibits a yellowish hue, suggestive of an older stellar population and reduced star formation. Moving outward from the core, there is a gradual decrease in surface brightness. The outer regions display a bluer tint compared to the core, possibly indicating the presence of some younger stars or ongoing, albeit low, star formation. The overall structure appears relatively undisturbed, lacking any obvious signs of recent major mergers or significant tidal interactions. The galaxy has an elongated shape, appearing roughly cigar shaped.
