This galaxy exhibits a generally smooth morphology with a high degree of central concentration. The light profile appears relatively featureless, lacking prominent spiral arms or a well-defined disk structure. The galaxy's shape is largely circular, suggesting an elliptical or lenticular classification. A subtle color gradient is visible, with the central region appearing slightly redder compared to the outer regions, possibly indicating an older stellar population towards the core. There is a slight indication of disturbance or interaction with neighboring galaxies. There are two faint neighboring galaxies that may be interacting with the primary galaxy.
