The galaxy presents a morphology consistent with a relatively smooth, featureless elliptical galaxy. It exhibits a somewhat flattened, "in between" shape, being neither perfectly round nor particularly elongated. There is no strong evidence of a prominent disk structure or spiral arms. The color profile indicates a concentration of light in the redder wavelengths, suggesting an older stellar population. No signs of on-going major mergers are immediately visible. The galaxy does appear to have a minor disturbance, with an uneven tail, and is moderately luminous.
