This galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge that gradually fades into an extended halo. The color profile suggests a population of older stars, with a yellowish hue dominating the core and outer regions. There is a general lack of discernible dust lanes or spiral arm structures. The galaxy's shape is largely spheroidal, with a slight deviation towards a more ellipsoidal form, indicating a degree of flattening. There is no visually obvious evidence of recent or ongoing major mergers or tidal disturbances. The galaxy appears relatively undisturbed and relaxed.
