The observed galaxy presents as a spiral type, viewed at a slight angle relative to face-on. The galaxy exhibits a bright, moderately sized central bulge. Faint spiral arms are present, although the morphology appears somewhat disturbed, hinting at a possible interaction or past merger event. There appears to be a prominent bar structure through the center of the galaxy. Star formation is estimated to be low. The galaxy's estimated physical size is approximately 3 kpc. The galaxy is of intermediate mass. The spiral arms are moderately wound. The arm count appears to be two, although this is difficult to determine due to the disturbances.
