The galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits a spheroidal morphology, with no obvious spiral arm structures. The light distribution suggests a relatively evolved stellar population, particularly in the central region, indicated by the yellowish hue. The outer regions appear bluer, potentially indicating younger stars or ongoing star formation. There is no indication of a major merger or significant tidal disturbance in the immediate vicinity. A small amount of irregularity in the outer envelope of the galaxy is observed. The galaxy is of intermediate size.
