The galaxy presents as a largely featureless elliptical object. It exhibits a concentrated, bright central bulge that gradually diffuses outwards. The overall color appears slightly redder in the central region, potentially indicating an older stellar population. Moving outwards from the core, the color shifts to a more bluish hue, suggesting the presence of a younger, possibly star-forming population on the outskirts, although no distinct spiral arm structures or star-forming regions are discernible in this imagery. The galaxy's shape is not perfectly spherical but rather somewhat flattened or elongated, tending towards a disc structure. There is no obvious evidence of tidal tails, strong gravitational lensing, or interaction with other galaxies.
