The galaxy presents as a somewhat elliptical, disk-like structure with a prominent central bulge. The core region exhibits a yellowish-gold hue, suggesting an older stellar population. Fainter, bluer regions are visible extending from the central bulge, hinting at possible recent star formation activity within the disk. The morphology appears relatively undisturbed, without any obvious signs of major mergers or significant tidal interactions. Overall, the galaxy appears to be in a relatively quiescent state. There is a subtle warp within the galaxy's disk, indicating a mild gravitational disturbance. The disk is not seen completely edge-on, but not face-on either.
