The galaxy presents an elliptical morphology, appearing largely smooth in structure with a concentrated central bulge. The light profile indicates a relatively even distribution of stars throughout, with a gradual decrease in intensity moving outward from the core. There is a subtle flattening, suggesting it is not perfectly spherical. There is a yellow hue indicating a population of older stars, implying low current star formation. There might be some evidence of minor tidal disturbances, but the general form shows that the object is relatively undisturbed. It appears relatively massive for a galaxy at its distance.
