The galaxy presents as a generally smooth, elliptical object, exhibiting a high degree of circularity. The core is intensely bright, displaying a concentrated distribution of light, while the light intensity decreases gradually towards the edges, creating a diffused halo. There appears to be a slight asymmetry in the outer regions. The overall color is slightly redder, indicative of a relatively older stellar population and limited ongoing star formation. The galaxy does not appear to be significantly disturbed, although there are subtle hints of minor irregularities. There are no visible signs of a prominent disk structure or spiral arms. The estimated size is approximately 6 kpc in radius, and is a luminous, massive system.
