The galaxy exhibits a spiral structure with a prominent bulge. The bulge appears moderately sized and is characterized by a yellowish hue, potentially indicating an older stellar population. The spiral arms are not tightly wound; rather they are more open and somewhat flocculent in appearance. There is evidence of at least two distinct spiral arms. The disk of the galaxy appears somewhat inclined relative to our line of sight. The overall color of the spiral arms is bluer than the bulge, suggesting ongoing star formation. There appears to be some irregularity in the disk, possibly indicating minor disturbances. There isn't a prominent bar structure visible through the galaxy's center. The object is of intermediate luminosity and intermediate physical size.
