The galaxy presents as a relatively smooth and elliptical object. It displays a high degree of central concentration with a bright, well-defined core. Moving outward from the core, the luminosity gradually decreases, suggesting an older stellar population. The galaxy appears somewhat elongated, deviating slightly from a perfect circular shape. There is no evidence of prominent spiral arms or significant dust lanes, and the overall color is consistent with an evolved galaxy that has little active star formation. There may be evidence of minor tidal disruption, but the shape appears largely undisturbed.
