The galaxy presents a somewhat elliptical morphology with a prominent, bright central bulge. The surrounding disk exhibits a bluer hue suggesting the presence of ongoing star formation, though the disk appears relatively smooth with only minor disturbances or irregularities. There is a possible, very minor interaction occurring, and no strong evidence of major merging events. The galaxy appears to be of intermediate mass. Considering the overall smoothness and color, it may be in a transition phase between a more actively star-forming state and a quiescent state.
