The galaxy presents as a lenticular or edge-on spiral structure. It exhibits a bright, yellowish central bulge, elongated along its major axis. A relatively faint, bluish disk extends outwards from the bulge, suggesting the presence of some young star formation activity. The light distribution appears smooth, possibly indicating an older stellar population with minimal dust obscuration in the bulge. The galaxy is significantly elongated, appearing cigar-shaped. There is no strong evidence of significant tidal disturbances or ongoing major mergers in the immediate vicinity, though minor irregularities cannot be ruled out based solely on this image. Overall, the galaxy appears to be relatively evolved, with a moderate level of ongoing star formation within the disk component.
