The galaxy presents as a lenticular or possibly an elliptical galaxy, viewed at an oblique angle. The object exhibits a central bulge that appears yellowish-white in color, indicating an older stellar population. A faint disk is suspected due to the elongated shape and presence of what might be spiral arm features. The outer regions fade gradually into the background, implying a lack of significant ongoing star formation in the outer regions. No obvious dust lanes are visible. Overall, the galaxy exhibits a smooth, diffuse appearance, with no signs of active galactic nuclei or major disturbances due to mergers. The morphology suggests a relatively evolved system.
