The galaxy presents as a relatively compact, elliptical structure. Its light profile suggests a high degree of central concentration, with a bright core diminishing outward to a more diffuse halo. The overall color appears to be on the redder side, indicative of an older stellar population and a lack of significant ongoing star formation. There is little evidence of spiral arm structure or prominent dust lanes. The object appears smooth and lacks irregular features, indicating a well-mixed system with minimal recent disturbances or mergers. The morphology suggests a galaxy that has undergone significant dynamical relaxation and is likely composed of primarily older stars.
