The galaxy presents as a spiral with a defined disk structure. Two prominent spiral arms extend from the central bulge, displaying a relatively loose winding pattern. The bulge appears moderate in size relative to the overall disk. A bar structure is suggested within the central region, exhibiting a strong presence. There does not appear to be any ongoing major merging activity, but minor disturbances are not excluded based on the morphology. The galaxy's red color indicates a presence of older stars.
