The galaxy presents as an elongated, cigar-shaped structure. Its morphology suggests it may be an edge-on spiral galaxy, though the image resolution limits definitive classification. The central region exhibits a bright, concentrated bulge, possibly indicative of an older stellar population. The galaxy displays a noticeable color gradient, shifting from bluer hues in the outer regions to redder tones toward the core. This color gradient is suggestive of active star formation in the disk and a higher concentration of older stars toward the galactic center. The overall structure does not show any obvious signs of major mergers or significant tidal disturbances, though some minor asymmetries cannot be ruled out. The galaxy's apparent smoothness supports the possibility of ongoing or recent minor interactions.
