The galaxy presents a generally smooth, elliptical morphology. There's a subtle, elongated structure observed, suggesting a shape somewhere between round and cigar-shaped, but closer to being in between. The central region exhibits a slightly reddish hue, potentially indicative of an older stellar population. Moving outwards, the galaxy displays a bluer color gradient, potentially indicative of some on-going star formation. There's no clear evidence of strong tidal features or major disturbances, although the asymmetry is noticeable. There are no visible spiral arms or distinct disk components.
