The galaxy presents as a lenticular or edge-on spiral morphology, appearing as an elongated central bulge with a distinct axis of symmetry. There is a general lack of clear spiral arm structure. The light distribution is centrally concentrated, and appears relatively smooth, with no prominent knots of star formation visible in the image. The galaxy displays a color gradient, shifting from a bluer hue at its core to a redder color towards its outer edges. The overall color suggests a moderate amount of older stellar populations. The high ellipticity indicates that the system is highly flattened. There is no clear evidence of a recent merger event or major tidal disturbance.
