The galaxy presents as a moderately inclined, disk-shaped structure. It exhibits a generally smooth morphology with a prominent central bulge, though some faint, diffuse features suggest a possible spiral structure. The central bulge is more yellow-white in color, hinting at an older stellar population. The outer regions of the disk are bluer, consistent with the presence of younger, hotter stars and possible ongoing star formation. The shape of the galaxy is elongated, leaning towards a cigar shape, and does not appear to be undergoing any major mergers or disturbances based on its largely undisturbed form.
