The galaxy appears as a somewhat diffuse object, exhibiting a dominant central bulge with a noticeable disk structure. The bulge shows a concentrated luminosity, appearing yellow to white, suggesting a population of older stars. The surrounding disk component, while present, shows hints of spirality. The disk is not sharply defined and exhibits a patchy distribution of light, indicating possible dust lanes. The general color profile suggests an evolved system with moderate star formation. There is a slight asymmetry visible in the outer regions of the disk, possibly indicating a minor interaction or disturbance.
