The observed galaxy presents a morphology consistent with a disk galaxy, likely of the lenticular type. The central bulge exhibits a smooth, concentrated luminosity profile, appearing relatively large and well-defined. Surrounding the bulge, a fainter disk component is visible. The disk appears primarily smooth with hints of spiral structure. The galaxy is viewed nearly face-on, as indicated by its relatively circular isophotes. The overall color suggests a stellar population that is relatively evolved. There are no obvious signs of ongoing major star formation, and the colors are consistent with an older population of stars. The outer regions of the galaxy become fainter, indicating a gradual decline in stellar density with increasing radius.
