The galaxy presents as a centrally concentrated, luminous object. It exhibits a largely smooth morphology, with a prominent central bulge that transitions into a broader, less defined disk. The bulge appears to be yellowish-white, suggesting a population of older stars. The surrounding disk is bluer in color, indicating the presence of younger stellar populations and ongoing star formation. The overall shape is predominantly round. There is no obvious evidence of spiral arm structure, bars, or major tidal disturbances, and it seems to be a relatively undisturbed system. The galaxy appears to be isolated, with no clear signs of interactions with other galaxies.
