The galaxy presents as a largely featureless elliptical or lenticular system. It exhibits a high degree of central concentration, with a bright, yellow-white core that dominates the overall luminosity. The galaxy displays a smooth, gradually diminishing radial profile, suggesting an older stellar population and a lack of significant ongoing star formation. The observed light distribution is roughly circular, with a slight tendency toward being rounded, indicating minimal signs of recent mergers or tidal disturbances. Based on the color indices, the galaxy's stellar population appears to be dominated by evolved stars. No spiral arms or significant dust lanes are visible. There are indications of minor disturbances, but the galaxy's structural integrity is mostly intact.
