The galaxy presents as a lenticular or early-type spiral morphology, exhibiting a dominant central bulge with a smooth, diffuse appearance. The color profile suggests a population of older stars, with a yellowish-orange hue dominating the bulge region. There's evidence of a faint disk structure surrounding the bulge, slightly elongated along its major axis. Subtle color variations within the disk suggest some degree of ongoing or recent star formation, with bluer regions indicating younger stellar populations. One side of the galaxy appears to show a tidal tail, which suggests a past interaction with another galaxy. Overall, the galaxy appears to be relatively massive, showing low specific star-formation rate, with its current rate concentrated in the disk region.
