The galaxy appears as a centrally concentrated object with a relatively smooth light distribution. The color profile suggests a moderate presence of young, blue stars, although the dominant light emanates from older stellar populations, giving it a somewhat yellowish overall hue. The galaxy shows a near round morphology. There are some hints of disturbances in its structure, such as faint, irregular features surrounding the main body, possibly indicating minor gravitational interactions or recent accretion events. The core of the galaxy is bright, suggesting a central concentration of stars. The overall shape lacks the distinct features of a spiral galaxy, pointing more towards an elliptical or lenticular type.
