The galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth morphology with a moderate degree of elongation. A central bulge region is evident, displaying a yellowish-orange hue suggestive of an older stellar population. Moving outward from the core, a fainter, more diffuse region is visible. The overall color gradients suggest a potential decline in star formation from the inner regions to the outer edges. There are possibly some minor disturbances, but the galaxy appears generally undisturbed.
