The galaxy appears to be an elliptical type. It presents a generally smooth and centrally concentrated light distribution. The central region appears to be a bright yellowish-orange color, potentially indicating an older stellar population. The light fades gradually outwards, transitioning to a slightly greenish hue in the outer regions. There is no clear evidence of spiral arms or a distinct disk structure. The galaxy has a moderately elongated shape, approaching a cigar-like appearance. There are no obvious signs of major mergers or strong tidal disturbances, although subtle irregularities in the outer halo might suggest minor interactions in the past. 
