The galaxy presents as a luminous, elliptical-like structure with a predominantly smooth morphology. Its core region exhibits a high concentration of light, suggesting a dense stellar population. The overall color profile indicates a relatively evolved stellar population, possibly with a diminished rate of ongoing star formation. A slight asymmetry in its shape might suggest a past minor interaction or internal disturbance. The apparent lack of prominent spiral arms or distinct dust lanes further supports classification as an early-type galaxy. Faint, diffuse extensions appear to emanate from the main body, hinting at a tidal interaction or residual star formation in the outskirts.
