The galaxy presents a primarily smooth morphology, with a concentrated central bulge that appears yellowish-orange in color. This likely indicates an older stellar population dominating the core. Moving outwards from the center, the galaxy's color transitions to a slightly bluer hue, especially on the bottom and right side. This might suggest the presence of some younger, hotter stars and ongoing star formation activity in the outer regions, although not overwhelmingly so. There's a slight elongation to the structure, suggesting it is not perfectly spherical, but rather somewhere in between an elliptical and a disk-like shape. There are some hints of minor disturbances present, but on the whole the system appears relatively undisturbed. This galaxy appears to be a rather massive object, with a relatively high rate of star formation activity.
