The galaxy presents as a relatively smooth, disk-like structure with a notable bulge. The central region exhibits a yellow-orange hue, possibly indicative of an older stellar population. Fainter, bluish components appear at the outer edges of the galaxy, possibly from more recent star formation. The galaxy shows an elliptical profile, with the major axis significantly longer than the minor axis, which suggests we are viewing a disk galaxy at an oblique angle. There is a possible slight disturbance in the morphology, potentially suggesting a minor interaction or merger event, although the overall structure appears relatively undisturbed. Overall, the galaxy seems to be a mid-mass galaxy, likely in a transition phase, with some ongoing star formation but a predominantly older stellar population.
