The galaxy presents a generally smooth, elliptical morphology. Its central bulge is a prominent, concentrated region exhibiting a yellowish-white hue, indicative of an older stellar population. Progressing outwards from the core, a more diffuse, blueish-tinted halo is observed. Subtle irregularities in this outer region suggest the presence of some minor disturbances and/or ongoing interactions. Overall, the galaxy demonstrates a well-defined structure with gradual transitions in color and luminosity from its center to the surrounding space.
