The galaxy presents as a somewhat diffuse elliptical structure. The core region displays a pronounced yellowish hue, suggesting an older stellar population. Moving outward from the core, there are hints of bluer regions, possibly indicating areas of recent or ongoing star formation, although these features are not sharply defined. The overall morphology lacks distinct spiral arm structure or a prominent bulge, leaning toward a more spheroidal shape with some irregularities in the outer regions, suggestive of potential tidal interactions or past merger events. There appears to be a faint, extended halo surrounding the main body of the galaxy.
