The galaxy presents as a relatively face-on spiral with a noticeable bar structure. The spiral arms are well-defined, tracing a mostly symmetrical pattern emanating from the central bar. Two dominant spiral arms are observed. The arms exhibit a medium winding, not too tightly wound nor particularly open. The bulge is moderately sized, contributing significantly to the overall light profile. No substantial distortions or tidal features are discernible in the image, suggesting the galaxy is not currently undergoing a major merger event. The galaxy exhibits a blue hue, indicating the presence of recent star formation. The nucleus appears bright, with the galaxy's color becoming redder towards the outer edges.
