The galaxy presents a lenticular or early spiral morphology, seen at a significant inclination. It exhibits a smooth, centrally concentrated light distribution, with a prominent bulge region displaying a yellowish hue, indicative of an older stellar population. Fainter, bluish light extends outwards from the central region, potentially associated with younger stars within a faint, disk-like structure. There is no strong evidence of distinct spiral arms, although a subtle, elongated asymmetry can be observed. There is no evidence of tidal disturbances or interactions with other galaxies in this image. Overall, the galaxy appears relatively undisturbed and evolved.
