The galaxy presents as a relatively compact, elliptical-like structure. It exhibits a smooth, somewhat amorphous morphology without readily discernible spiral arms or a prominent galactic disk. The color distribution suggests a dominant population of older stars, with a yellowish-red hue concentrated in the central regions. There is some suggestion of bluer regions. The overall shape is slightly elongated. No clear signs of tidal disturbances or ongoing major mergers are apparent, though subtle asymmetries may indicate minor gravitational interactions in its recent past. The galaxy appears to be well-defined and not particularly diffuse, indicating it is a mature system.
