The galaxy presents a primarily smooth morphology, with a high degree of central concentration. The light profile suggests a significant bulge component dominating the overall structure. While a disk component may be present, it is not readily apparent in this image due to the dominance of the bulge.

Color gradients indicate that the central region has a yellowish hue which is a signature of older stellar populations. Moving outward, there is a change to bluer colors, possibly indicating some regions of recent star formation. However, these regions are relatively faint and do not contribute significantly to the overall luminosity. Some minor disturbances within the galaxy are hinted at, but the overall form is not substantially disrupted. Therefore, this galaxy is likely undergoing only minor interactions or experiencing a low-level merger event.
