The galaxy presents as a generally smooth, elliptical-like structure. It exhibits a yellowish hue concentrated towards the center, suggesting an older stellar population dominating the core. There is a slight elongation, indicating it is not perfectly spherical. A fainter, diffuse component appears to be in close proximity to the main body, possibly a smaller galaxy undergoing a minor interaction or merger. There is little evidence of strong tidal tails or significant disturbances within the visible structure, suggesting a relatively relaxed state, although a subtle distortion cannot be ruled out based on this single image.
