The galaxy presents as a relatively smooth, centrally concentrated object with a roughly elliptical morphology. Its core exhibits a bright, yellowish-white luminosity, suggestive of an older stellar population dominating the central region. The luminosity gradually diminishes outwards, transitioning to a less defined, bluer halo. Faint, diffuse outer regions are visible, lacking distinct spiral arm structures or prominent dust lanes. There is a slight indication of possible minor tidal disturbances on the outskirts of the galaxy. The overall color suggests intermediate levels of star formation activity.
