The galaxy presents a generally smooth, elliptical morphology. Its light profile appears relatively uniform with no obvious spiral arm structures or distinct central bar. There is a slight elongation observed, and a shape between round and elliptical. The galaxy displays a color gradient, with a more pronounced reddish-yellow hue towards the central regions, suggesting an older stellar population dominating the core. Fainter blueish emission on the outer edges is apparent suggesting the presence of younger, star forming regions, which implies ongoing or recent star formation, albeit at a low rate. The galaxy does not appear to be undergoing any major merging events, but a minor disturbance in its morphology cannot be ruled out. Based on its overall appearance, this galaxy is likely a massive system.
