The galaxy presents as a smooth, centrally concentrated elliptical. It exhibits a spheroidal morphology with no discernible disk component. The galaxy is slightly elongated, deviating minimally from a perfectly circular shape. There is a suggestion of a weak tidal feature or minor disturbance in the galaxy's outer halo. Color gradients appear subtle, suggesting a relatively old stellar population throughout the galaxy, with little evidence of ongoing star formation. The light distribution is dominated by older, redder stars. The galaxy appears to be a relatively massive system.
