The galaxy presents a prominent spiral structure, exhibiting well-defined arms extending from a central bulge. These arms appear tightly wound, displaying a notable degree of symmetry. Dust lanes are visibly interwoven within the spiral arms, obscuring the underlying stellar population and contributing to a mottled appearance. The central bulge appears relatively moderate in size and exhibits a smooth texture. There's an indication of a possible bar structure crossing the central bulge, based on a subtle asymmetry in the distribution of light. The overall color profile suggests a significant population of older stars, especially in the bulge, however, the disk features bluer regions indicative of ongoing star formation. The galaxy demonstrates an elliptical form.
