The galaxy presents an elliptical morphology with a central bulge that appears bright and concentrated. The color profile indicates a relatively older stellar population, with a yellowish hue dominating the central region. There's a subtle indication of a disk-like structure extending from the central bulge, although it lacks well-defined spiral arms. The outer regions of the galaxy fade gradually into the background sky, suggesting a smooth density gradient. There appears to be some asymmetry in the outer profile, possibly indicating a minor gravitational disturbance or tidal interaction. Overall, the galaxy's appearance is consistent with a relatively massive system undergoing moderate star formation.
