The galaxy appears as a flattened, elliptical shape with a noticeable central bulge. The bulge exhibits a bright, concentrated luminosity. Moving outwards from the bulge, the galaxy displays a fainter disk or halo structure. There is some irregularity in the outer regions which may indicate that it is undergoing some sort of disturbance. There is a blueish color gradient that is visible within the disk or halo, which may indicate star formation activity. Overall, the galaxy lacks a well-defined spiral arm structure, and the light distribution appears relatively smooth.
