The galaxy appears as a centrally concentrated object with a generally smooth morphology. It exhibits a near-perfect circular symmetry in its overall shape, indicating a relatively undisturbed structure. The galaxy displays a color gradient, with a slightly bluer hue near the center transitioning to redder tones in the outer regions. This suggests possible variations in stellar populations or dust content across the galactic disk. There are no prominent spiral arms or bar features visible. There is no evidence of ongoing major merger activity. Subtle light variations and irregularities are present, but these appear minor and do not drastically disrupt the overall smooth profile.
