The galaxy presents a generally smooth and elliptical morphology. There is a central bright bulge, exhibiting a concentrated luminosity profile. Fainter, diffuse light extends outwards from the core region. A slight reddish hue is observed in the lower portion of the extended halo, possibly indicative of older stellar populations or dust obscuration within these regions. The overall structure appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. It is a galaxy with intermediate mass and star formation rate, based on its luminosity and color. The shape of the galaxy is mostly round. 
