The galaxy presents as a smooth, elliptical structure with a concentrated central bulge. Its overall shape is elongated, appearing cigar-shaped rather than perfectly spherical. The color gradient transitions from a yellowish core to bluer, fainter outer regions. There appears to be little evidence of spiral arms or distinct disk structures. No signs of major mergers or tidal tails are visible; however, a slight asymmetry suggests the possibility of minor disturbances or interactions. The galaxy's overall light profile suggests an older stellar population, with ongoing but relatively low levels of star formation.
