The galaxy presents a largely smooth, elliptical morphology. Its light profile is centrally concentrated, exhibiting a bright, yellowish core indicative of an older stellar population. The isophotes appear slightly elongated, suggesting a moderate ellipticity. A faint, diffuse halo surrounds the central region, fading gradually into the background. No distinct spiral arms, dust lanes, or significant substructure are apparent, indicating a lack of recent major merger events. There is very little evidence of on-going star formation, indicating the galaxy is likely quiescent.
