The galaxy presents a largely smooth morphology, appearing as a centrally concentrated spheroid of light. The luminosity profile suggests a relatively even distribution, lacking any distinct spiral arm structures or strong bar features. There is a subtle elongation visible, though the galaxy is mostly round, with a suggestion of a flattened disk component. The core region exhibits a yellowish hue, indicative of an older stellar population, while the outer regions are more blue, suggesting more active regions of star formation. Overall, the galaxy exhibits a generally undisturbed, evolved state, with only hints of past interactions or merging events. The galaxy does not appear to have any strong ongoing mergers or major tidal disturbances.
