The galaxy presents as a spiral type. Its disk is oriented close to face-on with respect to our line of sight. Prominent spiral arms are observed, tightly wound around a central bulge. The bulge appears moderately sized and of high surface brightness. The spiral arms show evidence of star formation, with some bluer regions visible. No strong bar is discernible, although subtle asymmetries within the central region cannot be ruled out as indicative of a weak bar structure. The overall morphology suggests a relatively undisturbed system, with no major signs of ongoing mergers, although there is evidence of a minor disturbance to its gravitational structure. The galaxy is faint and appears quite distant.
