The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge that gradually fades into a less dense halo. The color distribution suggests an older stellar population, with a dominant yellowish-orange hue in the central region. There may be faint indications of a disk-like structure, but this is not definitive. The overall morphology indicates that this galaxy is not currently undergoing any major merging events, although a minor disturbance cannot be entirely ruled out. The approximate size is moderate and would appear to be fairly massive, exhibiting moderate star formation activity.
