The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape is approximately elliptical, although it is slightly elongated. There's a bright central bulge, likely indicative of a substantial supermassive black hole. The color profile suggests the presence of both older stellar populations, contributing to the redder hues, and younger, bluer stars. The galaxy's outskirts appear to fade gradually into the background, with no obvious spiral arm structure or prominent dust lanes visible. Faint features indicate minor gravitational disturbances. Overall, this galaxy appears to be an elliptical galaxy, with a moderate amount of star formation occurring.
