The galaxy presents as a spiral type, exhibiting a significant disk structure. Spiral arms are clearly visible, though they appear somewhat flocculent. The galaxy's central bulge is prominent and appears moderately sized. The color profile indicates a mix of stellar populations. The bulge exhibits a yellower hue suggesting older, redder stars, while the disk shows bluer regions indicative of ongoing star formation. There is some evidence of a bar-like structure extending from the bulge. There is no apparent major disturbance, such as a major merger, though the galaxy is not perfectly symmetric.
