This galaxy appears to be a relatively smooth, disk-like system, viewed at a moderately inclined angle. The central bulge exhibits a yellowish-white color, suggesting an older stellar population. Traces of bluer regions are visible within the disk, hinting at the presence of younger stars and ongoing star formation, although the rates may be relatively low. The galaxy presents an elongated shape, with a hint of asymmetry, but does not appear to be undergoing any major merging events. Overall, the galaxy seems to be a stable system.
