The galaxy presents as a relatively faint, elongated, disk-like structure, exhibiting a cigar-shaped morphology. A central bulge appears present with a yellow-white hue, suggesting an older stellar population dominating the core. The disk, oriented at a steep inclination relative to our line of sight, displays subtle blueish tinges along its edges, possibly indicating regions of more recent star formation. The overall structure appears undisturbed, with no obvious signs of major mergers or tidal disruptions. The galaxy seems to be relatively isolated and well defined. There is a redder, more diffuse region near one edge. 
