The galaxy presents as a luminous, centrally concentrated object with an overall smooth appearance. Its morphology is predominantly elliptical, exhibiting a slightly elongated shape. The core region appears to be a bright yellow, indicating an older stellar population. The outer regions display a faint, diffuse halo with a reddish hue, possibly suggesting a lower metallicity or dust content compared to the core. There may be very weak indications of a disk-like structure, but it is very faint if present, not a spiral galaxy. There is no evidence of any recent major mergers or significant tidal disturbances affecting the object.
