The galaxy presents an elongated, cigar-shaped morphology. The light distribution suggests a relatively smooth structure, with a concentrated central bulge that exhibits a yellowish hue. The outer regions of the galaxy show a fainter, bluish tint that extends along the major axis, indicating the presence of younger stellar populations. There is no clear evidence of a spiral arm structure or significant dust lanes. The overall appearance suggests a galaxy undergoing or having completed a transition towards a more quiescent state, with moderate star formation activity in its outer regions. Some minor disturbances are possibly present, though no major mergers appear to be occurring based on the overall smooth nature of the galaxy.
