The galaxy presents an overall elliptical morphology, though there is some suggestion of a flattened or disk-like component. The light distribution is relatively smooth, with the highest surface brightness concentrated in the central region, giving the appearance of a bulge. Moving outward, the light fades gradually and more irregularly. There appears to be minimal evidence of spiral arm structures, but a slight asymmetry in the outer regions is visible. The galaxy is slightly elongated, with an axis ratio suggesting it is viewed at an intermediate inclination. The color is generally consistent across the galaxy, with the central region appearing more yellow, likely indicating an older stellar population. The outer regions are slightly bluer, which could point to ongoing star formation, albeit at a low level. There does not appear to be any evidence of a major ongoing merger, though there may be some minor disturbance in the morphology.
