This galaxy appears to be a relatively compact object, exhibiting a bright central bulge or core region. The light profile suggests a centrally concentrated morphology, with a gradual decrease in luminosity extending outwards. There are some suggestions of possible disturbances, but not strongly featured, as indicated by the relatively smooth light distribution. The color profile, shows a predominantly bluish hue in the central regions, indicating a potential presence of younger stellar populations. The outer regions seem to exhibit a more reddish color, hinting at a more evolved stellar population, or possible dust extinction. Overall, the galaxy presents a relatively elliptical shape.
