The galaxy exhibits a generally smooth morphology, with a radial concentration of light. The central region displays a distinct reddish hue, suggesting an older stellar population or significant dust obscuration. Surrounding this core, there's a broader, more diffuse halo or disk-like component with a bluer tint, potentially indicative of younger stars. While the galaxy appears primarily smooth, there might be some minor disturbances or faint tidal features detectable, but they're subtle and challenging to characterize without more detail. The shape seems to be predominantly elliptical with its roundness, but with hints of being in-between round and a more elongated shape. Overall, the galaxy is relatively isolated with no indications of ongoing major mergers, or interactions.
