The galaxy presents a predominantly smooth morphology, appearing largely featureless at this resolution. Its shape is approximately elliptical, with an axial ratio suggesting it is viewed at a significant inclination. The light distribution displays a clear concentration towards the center, indicative of a prominent bulge. The color gradient reveals a central region with a yellowish hue, transitioning to a bluer tint in the outer regions. This could suggest older stellar populations concentrated towards the center, with younger, bluer stars contributing more significantly in the outer disk. There is no obvious evidence of strong spiral arm structure or major ongoing mergers, but the slight asymmetry hints at possible minor tidal disturbances. Star formation appears to be occurring at a low rate. The overall appearance is consistent with an early-type spiral or lenticular galaxy.
