The galaxy presents a distinctly elongated, cigar-shaped morphology, suggesting it is viewed nearly edge-on. A central bulge is evident, appearing concentrated and yellowish-orange in color, which implies an older stellar population. Fainter, bluish-grey hues extend outward from the bulge, forming a disk structure. This faint, bluer light may indicate regions of more recent or ongoing star formation. Overall, the galaxy exhibits a relatively smooth appearance with no obvious spiral arm structure or signs of major interaction or tidal disruption. There is a slight asymmetry to the disk, with one side appearing slightly more extended or less defined than the other.
