The galaxy appears to be a single, relatively smooth structure, with a generally elliptical shape. It presents a radial color gradient, appearing more yellow-white towards the center and gradually becoming redder towards its outer regions. This color variation could suggest differing stellar populations, with older, redder stars dominating the outer regions, and younger, bluer stars concentrated towards the center, although this is not obviously supported by the image. There is no clear evidence of spiral arm structures or a distinct galactic disk; the light distribution appears more diffuse and spheroidal. No significant tidal tails or other signs of major merger events are evident. There may be a very subtle asymmetry in the overall shape, but this is not significant. The image resolution limits further morphological classification.
