The galaxy presents a predominantly smooth morphology. It appears relatively rounded in shape, exhibiting minimal disk-like structure and no obvious signs of ongoing major mergers or significant tidal disturbances. A central bulge is apparent, characterized by a concentrated luminosity profile that is less distinct in color compared to the more homogeneous, surrounding galaxy. There are no prominent spiral arms or distinct features such as dust lanes visible. The overall color suggests a population of older stars, with a low star formation rate.
