The galaxy presents as a lenticular or possibly an elliptical galaxy, elongated in shape. It exhibits a smooth, diffuse light profile, concentrated towards the center, with little evidence of spiral arms or distinct features. The central region appears yellowish-white, suggesting an older stellar population. Fainter, bluer hues are visible in the outer regions of the disk, possibly indicating some ongoing star formation. The galaxy is significantly elongated, with a high axial ratio, appearing cigar-shaped. There's no immediately obvious evidence of major mergers or tidal disturbances. Overall, the galaxy seems to be a relatively quiescent system.
