The galaxy presents a generally smooth, elliptical morphology with a high degree of central concentration. Its shape is moderately elongated, appearing more "in between" round and cigar-shaped. The light distribution suggests an older stellar population, with a color gradient indicative of a higher concentration of older, redder stars towards the core. No distinct spiral arms or prominent dust lanes are visible. There are no obvious signs of ongoing major mergers or significant tidal disturbances. The galaxy's overall appearance is consistent with that of an early-type galaxy, possibly an elliptical or lenticular galaxy seen at a slight inclination. Some minor asymmetry may be present in the outer regions but could also be a feature of image quality rather than the galaxy itself.
