The galaxy presents as a relatively smooth, elliptical-like structure with a noticeable elongation. Its color profile appears to be generally redder, with a yellowish hue, suggesting an older stellar population and possibly a lower rate of current star formation. There is a subtle central concentration of light that is not quite a core, and the outer regions fade gradually into the background sky. Irregularities or defined spiral arm structures are not apparent in this image. The morphology suggests this galaxy is likely an evolved system. There may be evidence of a minor disturbance or past interaction, considering the slight asymmetry in the outer isophotes.
