The galaxy presents a generally smooth and rounded morphology. There is a noticeable concentration of light towards the central region, suggesting a prominent bulge. The color appears to be yellowish-white, potentially indicating an older stellar population. No distinct spiral arms or bar structures are discernible. The galaxy exhibits a relatively compact structure with a lack of significant disturbances or tidal features, implying it is likely not undergoing major merger activity. Overall, the galaxy's appearance is consistent with an elliptical galaxy or a lenticular galaxy with a dominant bulge component.
