The galaxy presents as a relatively compact object. Its dominant feature is a central bulge, which appears nearly spherical, with a high concentration of older stellar populations exhibiting a yellowish-white hue. Surrounding the bulge is a fainter, bluer disk component. The disk shows some signs of structure, although details are blurred, it has areas of higher concentrations of star formation. The distribution of light in the outer regions of the disk appears somewhat irregular, possibly indicating minor gravitational interactions or internal disturbances. Overall, the galaxy exhibits a generally well-defined structure with a mixture of evolved and ongoing star formation.
