The galaxy presents as a spiral type, although the spatial resolution limits detailed morphological classification. The disk is not perfectly edge-on, with some inclination visible. Prominent spiral arms are observed. These arms are not tightly wound, but rather appear to be of medium pitch angle with only one arm prominent in this image. The central bulge is discernible, not appearing dominant, but also not negligible. There is some evidence of minor irregularities or disturbances in the disk, possibly indicative of an interaction or merger event. The overall color suggests a mix of stellar populations, with the bulge and the disk regions exhibiting varying hues, hinting at differences in age and composition.
