The galaxy presents as a spiral, viewed at a slight angle but not fully edge-on. It exhibits a prominent central bulge, with a yellow-orange hue suggesting an older stellar population. The disk surrounding the bulge displays spiral arms, traced by a bluer, more diffuse light, indicative of ongoing star formation. There appear to be some disturbances in the galaxy indicating a possible merger. The lack of very bright or distinct star-forming regions within the arms hints at a relatively moderate rate of star formation across the galaxy. Overall, the galaxy appears to be a moderately massive spiral galaxy.
