The galaxy presents a somewhat elliptical morphology, viewed at an oblique angle. A central bulge region is apparent, exhibiting a yellowish-orange hue, suggesting a population of older stars. Fainter, bluer extensions appear to emanate from the bulge along the major axis, potentially indicative of spiral arm structures or a disk component. There are hints of disturbances in the outer regions of the galaxy, such as asymmetries or distortions in the light distribution, possibly suggesting an ongoing or past interaction with another galaxy. Some regions of reddish hue outside the central bulge may indicate ongoing star formation. Overall, the galaxy exhibits characteristics intermediate between elliptical and spiral types, with possible evidence of past or current interactions affecting its morphology.
