The galaxy presents a generally smooth and rounded morphology. It appears relatively undisturbed, with no obvious signs of a recent major merger or tidal interactions. The central region exhibits a bright, concentrated luminosity, suggesting a prominent galactic bulge. There is a subtle color gradient visible, transitioning from a slightly bluer hue in the outer regions to a more yellow/red-shifted appearance toward the core. This may indicate older stellar populations dominating the central bulge, whereas more recent star formation could be occurring within the disk. The galaxy's shape leans towards a more elliptical classification based on the roundness and lack of distinct spiral arm features. The estimated size suggests it is of intermediate size and likely possesses a substantial mass, with limited recent star formation. The galaxy is likely approaching quiescence.