The galaxy presents as a centrally concentrated, elliptical object with a smooth, diffuse morphology. There is a prominent bulge region that transitions smoothly into the outer regions. The color profile suggests an aging stellar population, with a yellow-orange hue dominating the galaxy's core. There are hints of bluer tones in the outer disk, suggesting some ongoing, but low level, star formation. No spiral arms are visible. There are no strong signs of a major ongoing merger or tidal interactions; however, there may be minor disturbances in the galaxy's symmetry. The galaxy appears nearly round in projection, with a very slight ellipticity.
