The galaxy presents as a moderately sized, somewhat amorphous structure with a dominant central bulge. The bulge exhibits a relatively smooth, concentrated light distribution. Surrounding the bulge is a less defined disk component, showing faint, diffuse arms. There appears to be active star formation, most apparent on the far side of the galaxy, contributing to a slightly irregular shape. There is a moderate amount of dust, causing some obscuration and reddening of the light in the disk regions, but it does not affect the overall brightness significantly. The galaxy shows signs of a minor disturbance, indicating a possible past interaction or merger event.
