The galaxy presents as a spiral type, though the precise morphology is somewhat disturbed. The central bulge appears prominent and moderately sized, with a yellowish-orange hue, suggestive of an older stellar population. Emerging from the bulge are defined spiral arms, exhibiting a blueish tint, indicative of ongoing star formation activity. The winding of the spiral arms appears of moderate pitch, exhibiting a two-armed structure.

There are observable irregularities and distortions in the galaxy's overall form, possibly suggesting interactions or past merger events with other galaxies. There appears to be a low disturbance on the outer edges. The galaxy exhibits an apparent disk structure with an average size compared to other galaxies in the image. 