The galaxy presents as a centrally concentrated object, appearing largely featureless and smooth. It exhibits a slightly elongated, oblate shape. The core is a bright, reddish hue, possibly indicating an older stellar population. Surrounding the core is a more diffuse halo with a bluish tint, which might suggest the presence of younger stars and ongoing star formation. There is no clear evidence of spiral arms or a well-defined disk structure. Minimal tidal disturbances are visible, implying it is not undergoing any major merger events. Overall, this galaxy appears to be an elliptical galaxy with moderate star formation activity.
