The galaxy presents as a somewhat symmetrical, disk-shaped structure. It exhibits a prominent central bulge, appearing yellowish in color, suggesting an older stellar population. Surrounding the bulge, a fainter, bluer disk is observed. This blue hue indicates the presence of younger, hotter stars and ongoing star formation. The disk is not perfectly uniform; subtle variations in surface brightness hint at spiral arm structures, though these features are not sharply defined. The galaxy's overall structure appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. The galaxy is moderately luminous, with evidence of both old and young stellar populations.
