The galaxy presents as a centrally concentrated, smooth structure, likely an elliptical type. Its core exhibits a yellowish-orange hue, possibly indicating an older stellar population. The galaxy fades gradually into its outer regions. The overall shape appears more 'in-between' than circular, with a possible slight elongation. There is no obvious evidence of spiral arms, tidal tails, or strong dust lanes visible in the image. There is no indication of any ongoing major merger events; any disturbances appear minor.