The galaxy presents as a disk-shaped system viewed at a high inclination, appearing elongated with a cigar-like morphology. The central bulge region exhibits a higher surface brightness and a yellowish-white color, potentially indicating an older stellar population and a lower rate of star formation. The outer regions of the disk show a bluer hue, suggesting the presence of younger stars. The disk appears relatively smooth, lacking prominent spiral arm structures, suggesting a possible lenticular or early-type spiral classification. There is no obvious evidence of recent mergers or tidal disturbances based on the image. The overall structure hints at a relatively quiescent system with a dominant spheroidal component.
