The galaxy presents as a spiral system with a notable disk. The disk exhibits flocculent spiral arm structure, appearing somewhat patchy and not sharply defined. A central bulge is discernible, appearing as a concentrated region of luminosity with a yellowish hue, suggesting an older stellar population. The disk shows a bluer tint, indicative of ongoing star formation. There are some signs of minor disturbances, such as slight irregularities in the disk's outer regions, which may point to minor gravitational interactions. The galaxy's overall morphology is elongated, resembling an elliptical shape when viewed from our perspective. It is actively forming stars but on the lower end, possibly due to a larger fraction of older stars.
