The galaxy presents a generally smooth and rounded morphology, with no apparent spiral arm structure or bar. The central region exhibits a significantly brighter, more concentrated luminosity profile compared to the outer regions, suggesting a prominent galactic bulge. The color profile appears relatively uniform across the galaxy, with a slight reddening toward the core. This could be indicative of an older stellar population dominating the bulge, with ongoing star formation occurring at a low rate. There's no visual evidence of any major merger events or tidal disturbances affecting the galaxy’s structure. Overall, the morphology is consistent with an elliptical galaxy or a lenticular galaxy viewed nearly face-on.
