The galaxy presents as a somewhat elliptical or lenticular shape, with a smooth, diffuse light distribution. Its core region exhibits a concentrated, bright yellow-orange hue, suggesting a population of older stars. Moving outward from the center, the color transitions into a greenish-yellow as the light becomes more diffuse. There's no strong evidence of spiral arm structure or dust lanes discernible in this image. A slight asymmetry could imply a minor tidal disturbance or past merger event, though the overall structure appears relatively undisturbed. The outer edges of the galaxy fade gradually into the background, hinting at a large, extended halo. The colour profile of the disk appears more like a late stage spiral or elliptical galaxy, hinting at an older less active galaxy.
