The observed galaxy presents an elongated morphology, appearing as a flattened spheroid. The central region exhibits a high surface brightness, suggestive of a concentrated nucleus or bulge. A faint, extended halo of diffuse light surrounds the central region. The light distribution appears asymmetric, with a possible tidal feature or streamer extending from one side, which hints at a gravitational interaction or recent merger event. The color gradient from the center outwards suggests differing stellar populations, with the central region appearing more yellow and red, potentially indicating older stars, and the outer regions exhibiting bluer hues, implying the presence of younger, hotter stars. There also appears to be a possible secondary nucleus or enhanced region within the main body, indicating an ongoing or past interaction.
