The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, with a noticeable decrease in luminosity moving outwards towards the edges. The color is primarily a yellowish-white hue, suggesting an older stellar population and reduced active star formation. There is minimal evidence of spiral arm structure or dust lanes. The overall morphology appears undisturbed, with no apparent signs of recent major mergers or tidal interactions. There may be a slight distortion of the circular shape, giving it a slightly elongated, lens-like appearance.
