The galaxy presents as a luminous, elliptical-like object with a generally smooth appearance. The primary body exhibits a concentrated central region that diffuses outward, with a slightly ellipsoidal shape. There is evidence of a smaller, fainter, secondary concentration of light located proximal to the main body. The colour gradient shifts from redder hues in the region of the smaller light concentration to a warmer, yellow-white in the central and surrounding regions of the primary, more substantial galaxy body. This may indicate an older stellar population contributing to the overall luminosity. Overall, the galaxy lacks any obvious spiral arm structures and appears relatively undisturbed, although there may be some interaction with the smaller light concentration.
