The galaxy presents as a spiral type, though at a significant tilt to our line of sight. The central bulge appears relatively small and exhibits a yellowish-white hue, suggesting an older stellar population. The disk, viewed at an oblique angle, displays a bluer color, indicating active star formation regions. Two main spiral arms are discernible, though somewhat tightly wound. One arm appears more prominent, extending from the galaxy's main body. There is slight visual evidence of minor disturbances in the outer regions of the disk, without signs of an active merger event. Overall, the galaxy appears to be a well-defined spiral with ongoing star formation.