The galaxy appears to be a relatively smooth, centrally concentrated system. It is likely a lenticular or early-type spiral galaxy, based on its overall morphology and lack of prominent spiral arm structures. The color gradient suggests a slightly redder central bulge, indicating an older stellar population, and a bluer, more extended disk. There is only minor evidence of any ongoing interaction or merging activity based on the lack of morphological distortions in the galaxy. The apparent elongation suggests that the galaxy is viewed at an angle, with the disk not oriented face-on. The light distribution is fairly symmetrical. Overall, the galaxy presents as a relatively quiescent system with a moderate stellar mass and comparatively low star formation rate.
