The galaxy presents as a centrally concentrated object with a relatively smooth and diffuse morphology. The core exhibits a yellowish hue, suggesting a population of older stars. There is a slight extension to the upper and lower part of the object, however the shape generally appears to be between round and elliptical. No prominent spiral arms or distinct features such as dust lanes are discernible within the galaxy's structure, but some irregularities are seen near the central core. This suggests the possibility of minor internal disturbances. The overall color gradient indicates that star formation activity is low within the galaxy.
