The galaxy presents as a luminous, centrally concentrated object with a noticeable bulge. It exhibits a generally smooth, elliptical morphology with a slightly elongated shape. The light distribution suggests that the galaxy is dominated by an older stellar population. There might be a hint of a faint disk-like structure surrounding the central bulge, though it lacks distinct spiral arms. The galaxy does not show strong signs of active star formation, though some is likely present. There are no obvious tidal features or major disturbances, suggesting it is not undergoing a major merger event, but there may be minor disturbances.
