This galaxy presents as an elliptical system with a smooth, diffuse light distribution. It exhibits an elongated shape, displaying a cigar-like morphology. The central region shows a concentration of light, appearing brighter and denser than the outer regions. The color profile suggests a dominant population of older stars, with a reddish hue in the core transitioning to a slightly greener tint in the outer regions, potentially indicating the presence of some younger stellar populations or nebular emission. There is no apparent evidence of spiral arms, dust lanes, or significant star formation activity. The overall structure appears undisturbed, showing no signs of recent or ongoing merger events.
