The galaxy presents as a somewhat elliptical structure with a smooth light distribution. The central region exhibits a pronounced concentration of light, indicative of a bulge component potentially dominated by older stellar populations. The outer regions appear more diffuse, lacking distinct spiral arm structures or prominent star-forming regions. The color gradient shows a subtle reddening towards the center, supporting the presence of older, redder stars, and a slightly bluer periphery, hinting at younger stellar populations or ongoing, but low, star formation in the outer disk. The galaxy's overall morphology suggests a possible intermediate stage between a spiral and an elliptical galaxy, or potentially a spiral galaxy with tightly wound and unresolved spiral arms. There is very slight evidence of disturbance, but overall the galaxy is not undergoing a major merging event.
