The galaxy presents as a slightly inclined disk galaxy. The central bulge region appears relatively bright and featureless, suggesting an older stellar population. There are hints of spiral arm structure visible. The galaxy displays a general blueish-white hue, indicating the presence of some young, hot stars, but the color is not strongly pronounced. The galaxy's shape is elliptical and fairly regular. The image doesn’t clearly indicate any major merger events, but there are a few subtle asymmetries that may indicate some tidal disturbances or minor interactions. The estimated size suggests a galaxy on the smaller side. Overall, the galaxy appears to be a spiral galaxy that is likely not highly active in star formation.
