The galaxy presents a generally smooth morphology, exhibiting a flattened, elliptical shape, possibly tending towards lenticular. The light distribution is concentrated towards the center, with a bright central bulge that appears yellowish in color. This suggests a significant population of older stars in the nucleus. Fainter light extends outwards from the core, fading into the background sky. The disk or outer regions are less defined, and the overall color appears somewhat redder, which may indicate an older stellar population and/or the presence of dust obscuring bluer light from younger stars. There is no obvious evidence of spiral arm structures, active star formation regions, or any major ongoing merger activity within this galaxy based on the available imaging. The galaxy appears largely undisturbed and relatively evolved in its morphology.
