The galaxy presents a generally smooth, elliptical morphology. The light distribution appears centrally concentrated, with a gradual decrease in brightness towards the outer regions. There's no obvious presence of spiral arms or a distinct disk-like structure. The galaxy appears to be relatively isolated, showing no signs of significant tidal disturbances or ongoing major mergers with other galaxies. Minor irregularities or disturbances cannot be completely ruled out. The color indices suggest a redder overall population, potentially indicating an older stellar population or a significant dust content. The galaxy is neither perfectly round nor highly elongated, appearing somewhere between a circular and cigar shape. 
