The galaxy presents a generally smooth, elliptical morphology. It appears moderately luminous, exhibiting a concentrated central bulge that gradually fades into a diffuse halo. The color gradient transitions from a slightly redder hue in the core to a bluer tint in the outer regions. There is subtle evidence of a faint disk-like structure, though not sharply defined. Slight irregularities in the halo could suggest minor disturbances or past interactions, however, there are no obvious signs of an ongoing major merger. Overall, the galaxy appears relatively undisturbed.
