The galaxy appears to be a relatively smooth object. While it displays some features, it lacks a well-defined spiral structure. The morphology tends towards elliptical rather than a distinct disk galaxy. The shape appears somewhere between round and slightly elongated. It's possible it is in the process of a merger, as there seems to be some disturbance in the main structure. There is evidence of ongoing star formation, as indicated by the bluer regions within the galaxy, particularly in a small distinct region. The overall color profile suggests a mixture of stellar populations, with older, redder stars contributing to the core and arms, and younger, bluer stars concentrated in more active regions. It is a galaxy of intermediate mass. The specific star formation rate is relatively low, indicating that it is not undergoing a particularly intense burst of star formation.
