This galaxy appears to be a relatively small, disk-shaped galaxy, viewed nearly edge-on. It exhibits a slightly elongated, cigar-like morphology. There is a noticeable concentration of light in the central region, suggestive of a galactic bulge or core. The disk itself appears smooth with some evidence of faint, diffuse spiral arm structure. The galaxy displays a bluer hue, indicating the presence of younger stellar populations and ongoing star formation. There are no clear signs of major mergers or significant tidal disturbances in the immediate vicinity, although subtle irregularities in the disk may indicate minor interactions or internal processes.
