The galaxy presents as a moderately bright, elliptical-shaped object. Its light profile appears smooth, with a concentrated central bulge that diminishes outwards. The color distribution shows a dominant yellowish-white hue, suggesting an older stellar population with minimal ongoing star formation. The galaxy's structure lacks distinct spiral arms or prominent dust lanes. The overall morphology indicates a system that is likely spheroidal with a disk, potentially an elliptical galaxy, with intermediate roundness. There is no apparent sign of a major merger. There is an indication of a minor disturbance.
