The galaxy presents a flattened elliptical morphology. It exhibits a bright, concentrated central bulge, with the light gradually diminishing towards the outer edges. The radial light profile appears to follow a Sersic profile. The color gradient indicates a redder core compared to the bluer outer regions. The galaxy is slightly tilted with respect to our line of sight. There are no obvious signs of strong spiral arm structures, though there is some evidence of a disk component. Overall, the galaxy appears relatively undisturbed, without any strong tidal features or signs of a recent major merger. There may be some minor disturbances in morphology.
