The galaxy presents as a generally smooth, somewhat elliptical structure. A central bulge region exhibits a higher concentration of light, appearing brighter and more uniformly colored. Extending outwards from the central bulge is a disk, although it appears quite smooth. The color gradients are subtle, but suggest a higher blue luminosity in the outer disk regions compared to the yellowish central bulge. There is no definitive spiral arm structure visible in the image. The overall morphology is not indicative of a major ongoing merger, though there may be some minor disturbances in the outer regions. The galaxy appears to be relatively isolated, without any obvious nearby interacting galaxies.
