The galaxy presents a largely smooth, elliptical morphology. The light distribution is centrally concentrated, with a bright, somewhat indistinct nucleus, suggesting the presence of an older stellar population. The overall color of the galaxy appears slightly redder, further indicating a lack of significant ongoing star formation and a dominant population of evolved stars. The galaxy exhibits a slight elongation, deviating from a perfectly circular shape. Faint, diffuse extensions are visible, indicating that the outskirts of the galaxy may extend further than the main body, but its hard to say how large these extensions are.
