The galaxy appears to be a faint, relatively small object. It exhibits a diffuse, somewhat amorphous morphology. There is a slight indication of a disk-like structure, although it is not well-defined. Some slight asymmetry is observed, potentially indicating a minor gravitational interaction. The color suggests the presence of a population of older stars, though deeper observations would be required to confirm the stellar population. Overall, the galaxy exhibits characteristics that are not strongly indicative of a dominant classification, appearing as neither a clear elliptical nor a well-defined spiral, warranting further investigation to determine its evolutionary stage and dynamical state.
