The galaxy presents a generally smooth morphology, with a notable central bulge that appears bright and concentrated. The overall color profile suggests a mix of stellar populations, with the bulge exhibiting a yellowish hue, potentially indicative of older, redder stars. Surrounding the bulge, a fainter, bluer halo-like structure can be observed, suggesting the presence of younger, star-forming regions. There is a possible indication of a slight disk structure. There is a very slight hint of disturbance, though the galaxy appears to be relatively undisturbed. The galaxy appears to be a moderate to high mass system. Overall, the galaxy appears to be a system undergoing moderate star formation.
