The galaxy presents as a relatively smooth and elongated structure. Its central region appears brighter and exhibits a yellowish-white hue, suggesting an older stellar population. The outer regions of the galaxy display a bluer tint, indicative of younger stars or ongoing star formation. The overall morphology leans towards a flattened, cigar-shaped appearance, lacking distinct spiral arms or a pronounced central bulge. There is no visual evidence of major mergers or significant tidal disturbances affecting the galaxy’s structure, though there appears to be a slight asymmetry or minor perturbation in the outer regions. The apparent size suggests a substantial galaxy, with the overall light distribution being fairly concentrated towards the center.
