The galaxy appears to be an elliptical galaxy, generally smooth in texture without clearly defined spiral arms or a prominent disk. Its shape is largely spheroidal, with a high degree of roundness. Coloration indicates a higher concentration of older stars, with reddish hues and little evidence of active star formation. There is a high concentration of light towards the center of the galaxy, suggesting a bright central bulge. There are no apparent signs of tidal tails, ongoing mergers, or significant morphological disturbances, though some asymmetry can be observed. There is a faint indication of a possible outer halo or extended stellar population.
