The galaxy presents as a relatively smooth, elliptical structure. Its color profile indicates a redder core region, transitioning to bluer outer edges, suggesting a possible age gradient with older stellar populations concentrated in the center and younger stars in the outskirts. The galaxy exhibits an elongated shape, appearing somewhat cigar-like rather than perfectly spherical. There is no immediately apparent indication of strong tidal interactions or recent major merger events, though a subtle asymmetry or minor disturbance cannot be entirely ruled out at this resolution. Overall, the galaxy appears to be a relatively evolved system with a moderate level of star formation.
