The galaxy presents an elliptical morphology, with a smooth, concentrated distribution of light. A prominent, bright central bulge dominates the structure, exhibiting a yellowish-white hue suggestive of an older stellar population. The overall form indicates that the galaxy is generally symmetrical, lacking strong evidence of spiral arms or significant irregular features. There is a very slight indication of asymmetry, although not substantial enough to strongly suggest a recent major merger. The light distribution gradually fades towards the outer regions of the galaxy without any sharp cutoffs, indicating a diffuse stellar halo. Based on the color and morphology, the galaxy appears to be a mature system, possibly undergoing a low rate of star formation.
