The galaxy presents a primarily smooth morphology, suggestive of an elliptical or lenticular type. It exhibits a distinct central bulge with a bright, concentrated core. Surrounding the core, there is a noticeable disk-like structure, viewed nearly edge-on. This disk appears somewhat thin and shows subtle color variations, indicating varying stellar populations or dust distribution within the disk. The overall color of the galaxy leans towards the red end of the spectrum, which is consistent with a galaxy that has an older stellar population and a relatively low star formation rate. There might be indications of minor disturbances, but no strong signs of ongoing major mergers. The galaxy has an apparent elongation, deviating slightly from a perfectly circular shape.
