The galaxy presents an elliptical morphology, exhibiting a relatively smooth structure with no obvious spiral arms or distinct features. It is elongated in shape, appearing somewhat cigar-shaped. The central region displays a concentration of light, suggesting a prominent bulge or core. Color gradients are visible, with a more reddish or yellowish hue dominating the central region, gradually transitioning to a slightly bluer tint in the outer regions. This may indicate a mix of older stellar populations in the center and younger stars forming in the outer disk. There is no immediately apparent presence of tidal tails or strong distortions indicative of a recent major merger event, although a minor disturbance cannot be ruled out. Overall, the galaxy appears to be a relatively evolved system with a moderate redshift, suggesting significant distance.
