The galaxy presents as a relatively elongated, cigar-shaped structure. The central region exhibits a bright, concentrated bulge, displaying a yellowish-orange hue, which may indicate an older stellar population. A disk component is visible extending beyond the bulge along the major axis. The disk appears somewhat disturbed, possibly indicating past or ongoing interactions, although no distinct tidal tails or bridges are immediately obvious. The outer regions of the disk show bluer colors, suggestive of younger stars, and perhaps ongoing star formation. The overall appearance is moderately smooth, but with subtle features hinting at underlying structure.
