This galaxy presents as an object of intermediate size, exhibiting a somewhat elongated morphology. The central region displays a high surface brightness, appearing nearly uniform and unresolved in this image. Moving outward from the core, the light profile diffuses gradually into a fainter, more extended halo. There is a hint of structure within the halo, potentially indicating the presence of a disk. The color appears relatively homogenous, with a subtle bluer tint observed in the outer regions compared to the more neutral core, perhaps hinting at ongoing star formation in those outer regions. The galaxy appears relatively undisturbed, with no obvious signs of a recent major merger event or strong tidal interactions. However, the presence of subtle asymmetries and the potential disk-like structure warrant further investigation to determine if minor disturbances have occurred. 
