The galaxy appears to be an elliptical galaxy with a smooth, spheroidal morphology. The light distribution is centrally concentrated, exhibiting a diffuse, yellowish-orange hue. There are potentially minor indications of disturbance, potentially suggesting an ongoing interaction or recent merger event with a smaller companion.

The estimated size of the galaxy is approximately 7.7 kiloparsecs in radius. The galaxy is relatively luminous, with an absolute magnitude that places it among the brighter galaxies. The estimated mass of the galaxy is substantial, being on the order of 10^11 solar masses.

Star formation activity is relatively low within the galaxy. This is consistent with the dominant population of older stars typically found in elliptical galaxies.
