The galaxy presents as a relatively smooth, centrally concentrated object with a largely homogenous appearance. The morphology indicates a likely elliptical galaxy, exhibiting minimal features such as spiral arms or significant dust lanes. The light is centrally concentrated, with a diffuse halo. There are no signs of tidal disturbances or other strong interactions with neighboring galaxies. The color suggests some recent star formation, as indicated by the presence of bluer light. The majority of light emitted by the galaxy seems to be clustered toward the center, with a decrease in brightness as one looks towards the periphery. 
