The galaxy presents as a spiral with a discernible disk structure. There are indications of well-defined spiral arms emanating from the central region. The central bulge is prominent and appears yellow, indicating a population of older stars. The spiral arms exhibit a bluer hue, suggesting ongoing star formation. The disk is not viewed edge-on, but rather at an angle.

There is noticeable asymmetry and distortion in the spiral arms. A possible interaction or minor disturbance appears evident. The galaxy's structure is suggestive of a system undergoing or having recently undergone a merger event, possibly involving a smaller companion galaxy, or a tidal interaction. There is no sign of a strong central bar, the bulge appears to be moderate in size.
