The galaxy presents as an elliptical morphology, appearing largely smooth in texture. The shape is somewhere between round and elongated, but mostly in between those categories. There is a noticeable color gradient from the core to the outer regions. The central region exhibits a yellowish-white hue, suggesting an older stellar population. The outer regions show hints of bluish light, possibly indicative of more recent, albeit subdued, star formation activity. There is no significant evidence of ongoing mergers or major disturbances, although a minor disturbance is not out of the question. The galaxy possesses an apparent magnitude that is consistent with it being a luminous galaxy.
