The galaxy presents as a centrally concentrated system, appearing largely smooth in morphology. The light distribution indicates a spheroidal shape, closely approximating a circular form. There is a bright central region which may indicate an active galactic nucleus or a dense concentration of stars. The galaxy's color exhibits a somewhat blue tint, suggesting the presence of a young, hot stellar population, although the overall smoothness suggests that active star formation is not vigorous. There are no prominent spiral arms or significant dust lanes visible. There is no evidence of any ongoing major mergers or tidal disturbances in the immediate vicinity of the galaxy.
