The galaxy presents as a generally smooth and rounded structure. There's a pronounced central bulge, appearing significantly brighter and more concentrated than the outer regions. This bulge exhibits a yellowish-white hue, suggesting a population of older stars. Extending outwards from the bulge is a fainter, more diffuse disk. The color of the disk appears slightly bluer, potentially indicating the presence of younger stellar populations and ongoing star formation, though at a low rate. No distinct spiral arms or bar structures are readily apparent. There might be some minor disturbances or subtle features in the outer regions, but no major interactions or mergers are readily apparent. Overall, the morphology suggests that this is likely an early-type galaxy, possibly an elliptical or lenticular galaxy.
