The galaxy presents as a largely featureless elliptical or lenticular system. The central bulge region exhibits a concentrated luminosity, appearing smooth with a yellowish hue. This suggests a dominant population of older stars. Moving outward from the core, the light gradually fades, and there are minimal signs of spiral arms or dust lanes. The shape is close to being in between round and elliptical. There is no visual evidence of any ongoing major merger activity or tidal disturbances. The galaxy is observed to be generally isolated. The red color in the galaxy suggests a low star-formation rate.
