The galaxy presents as a relatively bright, elliptical structure with a smooth, diffuse appearance. It exhibits a concentrated central bulge that transitions into a broader, less dense halo. The core region appears slightly yellowish, perhaps indicating an older stellar population or dust obscuration. A subtle disk-like structure is hinted at, oriented approximately horizontally in the image, although it lacks the distinct spiral arms typically associated with disk galaxies. Faint bluish hues are observed in the outer regions of the galaxy, potentially suggesting the presence of younger, hotter stars, or it could be a result of how the image has been processed. There is no visible evidence of ongoing major mergers or tidal disturbances and there is no dust lane.
