The galaxy appears to be a relatively compact object, exhibiting a smooth, elliptical morphology. There is little to no evidence of spiral arms or a prominent disk structure. The light profile seems concentrated towards the center, with a gradual decrease in intensity moving outwards. The color indices suggest that the galaxy may be dominated by an older stellar population, appearing redder than typical spiral galaxies. There are no signs of tidal disturbances or ongoing mergers, and the galaxy appears to be relatively isolated. Its overall shape suggests an oblate spheroid, exhibiting a slight deviation from perfect circularity. Based on its apparent size and estimated distance, the galaxy is likely a medium-sized galaxy. Star formation is not readily apparent, potentially indicating a quiescent or passively evolving system.
