The galaxy presents as a fairly smooth, elliptical-like structure. It appears elongated, exhibiting a cigar-like shape. The central region shows a higher concentration of light, indicative of a bulge or core. The color is primarily yellowish-orange, suggesting an older stellar population. There is a subtle color gradient, with the outer regions appearing slightly bluer compared to the core, possibly due to the presence of younger stars in the disk. There is no clear evidence of spiral arms or significant dust lanes within the resolution of the image. The overall morphology suggests that it is most likely an elliptical galaxy. There are no immediately obvious signs of any major ongoing merger events, though a minor disturbance or interaction cannot be entirely ruled out.
