This galaxy presents as a spiral type, viewed at an oblique angle. A prominent central bulge exhibits a yellowish hue, indicative of an older stellar population. The spiral arms are moderately wound and discernible, displaying a bluer color, suggesting ongoing star formation. There appears to be at least one other nearby object which could be a companion galaxy. There is also the hint of a faint tidal stream that is disrupted suggesting that the galaxy may be in the process of merging with one or more objects.
