The galaxy presents a clear disk-like structure indicative of a spiral galaxy, but exhibits only a moderate inclination relative to our line of sight. Well defined spiral arms appear present. The central bulge appears prominent and relatively bright, though not overwhelmingly dominant, suggesting a moderate bulge size. Faint traces of color variations within the spiral arms suggests ongoing star formation. The spiral arms appear tightly wound around the bulge. Overall structure looks largely undisturbed, without evidence of ongoing major mergers or significant tidal disruptions. The stellar population appears relatively old. The absence of major disturbances and the presence of a well-defined disk suggest a relatively stable, well-formed system.
