The galaxy presents as a somewhat flattened elliptical shape, observed nearly edge-on. It is dominated by a bright, relatively smooth central bulge, with a high concentration of light. Fainter, diffuse light extends outwards from this core along the major axis. There is evidence of a faint disk structure. No strong spiral arms are visible, and the galaxy lacks prominent dust lanes or active star-forming regions. There may be minor disturbances present in the morphology of this galaxy. The overall color gradient suggests a relatively older stellar population. It appears to be undergoing a merging event.
