The galaxy presents as a generally smooth, elliptical object. Its overall shape is quite round, with a high degree of central concentration. The core appears bright and yellowish, potentially indicating an older stellar population. There is little evidence of spiral arm structure or significant dust lanes. No major mergers or tidal disturbances are visible. There is a suggestion of a very faint, diffuse halo or extended envelope, with an apparent radius of approximately 3 kpc. Star formation is most likely low. Overall, this galaxy appears to be a fairly evolved, quiescent system.
