The galaxy presents as a relatively compact and luminous object. It appears to be largely spheroidal in shape, with a smooth, diffuse light distribution and a high degree of central concentration. There is a subtle color gradient from the core of the galaxy outwards, suggesting a possible transition in stellar populations or dust content. No obvious spiral arm structures, bars, or significant dust lanes are discernible in the image. The overall morphology indicates a possible early-type galaxy, likely elliptical or lenticular. There may be minor disturbances in the galaxy's structure, but a major merger event is unlikely.
