The galaxy presents as a moderately luminous object with a relatively smooth, elliptical morphology. The core region exhibits a concentrated brightness, suggesting a significant stellar density. A subtle, diffuse halo extends outwards from the core, gradually fading into the background sky. The overall color profile suggests an older stellar population, with a noticeable absence of bright, blue star-forming regions. Faint hints of possible substructure or tidal features are present in the outer regions, possibly indicating past minor interactions or mergers. The galaxy displays an approximate size of 4 kpc.
