The galaxy presents a generally smooth morphology, with a centrally concentrated spheroid. The shape is elongated, approximating a cigar shape rather than a perfect circle. It exhibits a moderate inclination relative to the observer. There is a possible subtle disk component present, but it is not clearly defined. Color gradients are observed, with a whiter-yellow hue dominating the core region, transitioning to a bluer color in the outer regions, indicative of a possible older stellar population in the center and younger in the periphery. No signs of major mergers or significant tidal disturbances are apparent. The galaxy shows no prominent dust lanes or distinct spiral arm structures, suggesting a relatively quiescent state. Overall, the appearance is consistent with an early-type galaxy, possibly an elliptical or lenticular type. The star formation rate appears to be on the lower end.
