The galaxy presents a largely smooth morphology, with a dominant, rounded central region. There is some evidence of faint, extended features or a possible disk-like structure, though these are much less prominent than the central bulge. The galaxy appears to be undergoing some level of interaction or disturbance, indicated by a slight asymmetry in its overall shape and the presence of possible tidal features or minor disturbances. The color distribution suggests a relatively blue central region, indicative of active star formation, with perhaps slightly redder colors in the outer regions, potentially indicating an older stellar population or dust obscuration. Overall, the galaxy appears to be an intermediate-mass system exhibiting both characteristics of an elliptical galaxy and a spiral galaxy.
