The galaxy presents as a relatively smooth, elliptical morphology. There is little to no evidence of spiral arms or a distinct disk structure. The light distribution appears fairly uniform across the galaxy's body, with a gradual decline in brightness towards the edges. The overall shape is nearly circular, lacking significant elongation or asymmetry. I detect no signs of major mergers or tidal disturbances. There may be evidence of minor disturbances or a faint, diffuse halo surrounding the galaxy. The color is consistent with an older stellar population, indicating a relatively low star formation rate. 
