The galaxy presents as a relatively smooth, disk-like system with a central bulge. The bulge region appears yellowish, suggesting an older stellar population with fewer hot, young stars. The disk component exhibits a slight inclination, revealing a flattened structure. There is a subtle color gradient from the bulge outwards, shifting toward slightly bluer hues, potentially indicating some ongoing star formation in the outer regions. The overall morphology suggests a disk galaxy with a dominant bulge component, where star formation rates are likely declining. There is no evidence of any significant tidal disturbance, such as extended tails or shells.
