The galaxy presents a moderately disturbed morphology, possibly indicative of a recent or ongoing interaction. A dominant central region exhibits a somewhat smooth appearance. Faint extended features are present, though their precise nature is difficult to ascertain. The galaxy shows a slight overall blue tint which suggests the presence of younger stars and ongoing star formation, though at a relatively low rate. The size of the galaxy is relatively compact. There may be evidence of dust lanes or patches obscuring the light from the stars, but the image resolution limits a definitive conclusion.
