The galaxy presents as a relatively smooth, elliptical structure. The light distribution is centrally concentrated with a gradual decrease in intensity outwards. There is a slight elongation to the shape, possibly indicating a mild cigar-like form or a disk seen at an angle. No distinct spiral arms or prominent dust lanes are discernible in the image. The galaxy's color appears yellowish-white, suggesting an older stellar population dominates its composition. There's no visual evidence of ongoing major mergers or significant tidal disturbances. A slight asymmetry may suggest a minor interaction, but the overall structure appears relatively undisturbed. The galaxy appears to be a fairly mature system based on its morphology and color.
