The galaxy presents a smooth, elliptical morphology. It exhibits a concentrated central bulge that graduates outwards to a diffuse halo, with no apparent spiral arm structures or dust lanes visible at this resolution. The color profile indicates a generally older stellar population, evidenced by its reddish-yellow hue. No signs of active galactic nuclei features or tidal disturbances are readily apparent, suggesting a quiescent state. The galaxy's structure appears relatively undisturbed, with no strong indications of recent major merger events.
