The galaxy appears as a somewhat elongated, centrally concentrated object. Its overall color is suggestive of an older stellar population, with a yellowish-white hue dominating its visual appearance. There is little evidence of distinct spiral arm structure or prominent star-forming regions; the light distribution appears generally smooth. The galaxy's shape leans towards an elliptical morphology but does show signs of some disclike structure, meaning it is likely a lenticular galaxy. There is some evidence of mild disturbance; this is difficult to confirm given image quality but is possibly a minor interaction or merger.
