The galaxy presents as a somewhat elongated, elliptical morphology. The light distribution appears generally smooth and centrally concentrated. The galaxy exhibits a yellowish hue, potentially indicative of an older stellar population. There is a faint suggestion of a disk, although no spiral arm structure is clearly discernible. A possible minor disturbance is present, although the central body of the galaxy remains relatively undisturbed. There does not appear to be a strong ongoing star formation rate within the galaxy, as inferred from the older stellar populations. Based on its color and form, the galaxy likely has a large mass.
