The galaxy presents as a relatively smooth, elliptical structure. It exhibits a dominant central bulge with a concentrated, bright core. The overall color appears yellowish-orange, suggesting an older stellar population with minimal ongoing star formation. There is a slight elongation to the galaxy's shape, deviating marginally from a perfect circularity. No distinct spiral arms or prominent dust lanes are discernible. The galaxy appears isolated, with no immediate signs of tidal interactions or merging activity with other galaxies. The light distribution is centrally concentrated, fading gradually towards the outer edges. The galaxy's morphology is suggestive of a passively evolving system.
