The galaxy presents as a generally smooth, centrally concentrated object. It exhibits a slightly elliptical morphology, with a roughly round overall shape. The central region displays a yellowish hue, suggestive of an older stellar population. Progressing outwards from the core, the color transitions to a slightly bluer tone, which hints at the presence of younger stars. There is no apparent spiral structure, nor are there any prominent dust lanes visible. Faint, somewhat amorphous extensions can be perceived on opposing sides, but they do not clearly indicate any major ongoing mergers or interactions, merely minor disturbances perhaps from recent interactions. The overall impression is that of a relatively quiescent galaxy.
