The galaxy presents as a spiral type, exhibiting a prominent bar structure traversing its central region. Two well-defined spiral arms emanate from the ends of the bar, tightly wound, and extending outwards into the galactic disk. The bulge appears moderately sized, contributing significantly to the overall luminosity of the galaxy's core. The disk is the predominant feature, with the spiral arms displaying a somewhat flocculent morphology. There are no indications of significant tidal disturbances or major merger activity, although a minor asymmetry suggests potential minor interaction or internal dynamics. The colour gradient suggests active star formation regions along the spiral arms, though this feature is not immediately apparent. Overall, the galaxy appears to be a barred spiral system with a fairly standard morphology for its type.
