The galaxy presents a generally smooth morphology. It exhibits a somewhat rounded shape, with a color gradient indicative of varying stellar populations. The central region appears more concentrated and exhibits a yellowish hue, suggesting a population of older, redder stars. Moving outwards from the core, the color transitions slightly, indicating the presence of some younger, bluer stars, though the overall color profile suggests that older stars are dominant. There is no clear evidence of spiral arms or a distinct disk structure. The overall structure is somewhat amorphous. There may be some minor distortions in the outer regions, which could be signs of past interactions or minor mergers. No major disturbances or ongoing mergers are evident in this image. Overall, the galaxy appears to be a relatively evolved system.
