This galaxy presents as a luminous, elongated structure, with a notably smooth, featureless appearance. It appears to be a relatively isolated system. The color distribution is non-uniform. A bright, yellowish-white core region dominates the central area, suggesting a high concentration of older stellar populations. The outer regions of the galaxy exhibit a slightly bluer hue, hinting at the presence of younger stars and ongoing, but subdued, star formation. There is a slight disturbance on the left side of the galaxy which could be an artifact, however it may also be a sign of an early merging event. The overall morphology suggests an elliptical galaxy, likely undergoing passive evolution given the smoothness of the disk and lack of apparent recent major merger activity.
