The galaxy presents an overall elliptical morphology, with a smooth, diffuse light distribution. The central region exhibits a high concentration of light, appearing as a bright, slightly elongated core. Moving outward from the core, the light intensity gradually decreases, lacking any distinct spiral arm structures or prominent dust lanes. There is a subtle color gradient, with the central region appearing more yellow/orange, possibly indicating an older stellar population. The outer regions appear slightly bluer, though not definitively indicative of ongoing star formation. Some minor tidal disturbance may be present.
