The galaxy presents as an elongated, moderately luminous system. Its morphology appears predominantly smooth, suggesting a relatively evolved stellar population and a lack of significant ongoing star formation. The central region exhibits a concentration of light, potentially indicative of a bulge component. Faint blue tinges emanate from the outer regions, suggestive of some younger stars and/or star-forming regions distributed within a disk. There is no evidence of major mergers or significant tidal disturbances. The galaxy possesses a noticeable disk structure, though it is not sharply defined, and exhibits an overall elliptical shape, indicative of a system that may be intermediate between a pure elliptical and a spiral galaxy.
