The galaxy presents as a relatively large spiral galaxy, viewed at an oblique angle. There is evidence of a prominent disk structure. The disk appears to be undergoing some level of disturbance, possibly due to interactions or internal dynamics. A significant portion of the light from the galaxy seems to be concentrated in what appears to be the bulge region. The light from the galaxy is relatively bright, indicating a substantial population of stars and ongoing processes within it. Furthermore, the presence of color variation suggests active star formation regions. The spiral arms appear to be somewhat loosely wound.
