The galaxy presents a generally smooth morphology, appearing as a concentrated central region with a less defined, more diffuse halo. The galaxy exhibits a somewhat elongated, cigar-shaped form, deviating from a perfectly circular structure. It displays an orange hue. There is an indication of a possible minor disturbance to the structure; this could be from a small merger that it is undergoing. The estimated stellar mass of the galaxy is significant, implying that this object contains a large population of stars. The galaxy shows evidence of ongoing star formation activity.
