The galaxy presents as a relatively smooth, elliptical or lenticular structure. The central bulge is prominent, displaying a concentrated, yellowish-white light profile suggestive of an older stellar population. There is little evidence of spiral arms or significant dust lanes within the observable morphology. The color gradients transition subtly outward, and the overall shape deviates slightly from perfectly circular, tending towards a more oblong or slightly flattened appearance. There is an additional, smaller object close to the main body of the galaxy, appearing as a faint, diffuse region of blue light, possibly indicative of tidal interactions or ongoing minor merger activity. The overall structure hints at a system that may be in the later stages of its evolution, with relatively low star formation activity, exhibiting a smooth morphology. 
