The galaxy presents an elongated, cigar-shaped morphology, suggesting it may be either an elliptical galaxy or a spiral galaxy viewed edge-on. It exhibits a prominent, bright central bulge that appears yellowish in color, indicative of an older stellar population. Fainter, bluer regions are visible along the outer edges of the galaxy, hinting at the presence of younger stars and ongoing star formation, but at a low rate. No distinct spiral arms are visible; however, the faint blue hue suggests the presence of a disk-like structure. There is no significant sign of any major disturbance or recent merger event. The overall smoothness of the galaxy suggests a relatively evolved system. 
