The galaxy presents as a relatively smooth, centrally concentrated object, appearing nearly round in projection. There is a noticeable radial color gradient, transitioning from a yellowish core to fainter, slightly bluer outer regions. This suggests a possible decline in stellar age and/or metallicity with increasing distance from the galactic center. Faint features may be present, perhaps indicative of a weak disk, however, there is no substantial evidence for spiral arms. The galaxy does not appear to be undergoing any major merging events or strong tidal disturbances, though a slight asymmetry might indicate minor past interactions. The overall morphology indicates this galaxy is most likely a lenticular or elliptical galaxy, where star formation is suppressed. 
