The galaxy presents as a moderately luminous, elliptical-like structure. Its central region is characterized by a high concentration of light, appearing almost spheroidal. Progressing outward from the center, the luminosity gradually decreases, forming a diffuse halo. The object exhibits a generally smooth texture with minimal discernible features such as spiral arms or prominent dust lanes. Faint blue hues are visible in the outer regions of the galaxy, potentially indicating the presence of younger stellar populations or ongoing, though subdued, star formation. There is a very subtle elongation to the object's shape; it isn't quite circular, but it does not appear to be significantly disturbed or undergoing a major merging event. The overall impression is that of a relatively quiescent galaxy with a dominant older stellar population.
