The galaxy presents a generally smooth, rounded morphology. There is a prominent central bulge, concentrated in a yellowish hue, suggesting an older stellar population. The surrounding regions are less concentrated and exhibit a bluer tint, which could be caused by the presence of younger, hotter stars. There is no obvious spiral arm structure or strong dust lane features that would classify it as a spiral galaxy. The light distribution from the center outwards falls gradually, with no indication of a significant ongoing merger event, though subtle disturbances are possible. Overall, this galaxy appears to be an elliptical galaxy.
