The galaxy presents as a spiral with a moderate inclination relative to our line of sight. Faint spiral arms are discernible, exhibiting a somewhat flocculent structure. A central bulge is present, appearing neither overly dominant nor negligible in size. Within the central region, light appears to be concentrated. The galaxy does not appear to be undergoing any major merging events, although there might be some minor disturbances present. A faint, almost indiscernible, bar structure could be present in the center. The galaxy's color is generally bluish, especially in the less dense regions.
