The galaxy presents as a relatively smooth, elliptical morphology. There is a bright, concentrated central bulge. The light gradually decreases outwards from the center, displaying a shallow gradient, indicating a high Sersic index. The galaxy exhibits a moderate ellipticity; it is not perfectly circular, but not highly elongated. The galaxy's color profile appears consistent across its surface. The overall color is biased towards the redder end of the spectrum. No distinct spiral arm structures or significant dust lanes are apparent. There is no clear sign of recent major merger activity, although a subtle perturbation in the outer isophotes cannot be ruled out at this resolution. The galaxy's stellar population is likely dominated by older stars with low star formation activity.
