The galaxy presents a generally smooth morphology, with a bright, concentrated central region that appears yellowish. There is little evidence of distinct spiral arms or a pronounced disk structure. The light distribution suggests a spheroidal shape, possibly an elliptical galaxy or a lenticular galaxy viewed face-on, with the central bulge dominating the overall appearance. A faint, diffuse halo surrounds the central region, fading gradually into the background. There is a hint of some subtle disturbances, though these do not drastically disrupt the overall smoothness, suggesting potential minor gravitational interactions. The galaxy's light profile indicates a mature stellar population, given the redder hues. It is likely a relatively massive system. The overall structure seems consistent with a galaxy transitioning towards a more quiescent state in terms of star formation.
