The object presents as a spiral galaxy, viewed at an oblique angle. The spiral arms are well-defined, extending outwards from a central bulge. These arms show prominent blue regions indicative of active star formation. The bulge has a moderate size relative to the overall galaxy structure. No signs of major merger events or tidal disturbances are apparent. A slight asymmetry may suggest a minor interaction or disturbance. There is potential evidence of a bar structure.
