The galaxy presents a predominantly smooth morphology. It exhibits an elongated, cigar-like shape, suggesting it may be an elliptical galaxy or a lenticular galaxy seen edge-on. The central region displays a yellowish hue, potentially indicating an older stellar population. Fainter bluish fringes are visible at the outer edges of the galaxy, possibly regions of more recent star formation, though the smooth overall structure suggests this is not a dominant feature. There is no visible evidence of spiral arms or major disturbances indicative of an ongoing merger. The galaxy appears relatively isolated in this image.
