The galaxy presents a largely smooth morphology. It appears centrally concentrated with a bright, somewhat diffuse core. There is a subtle ellipticity to the overall form, deviating slightly from a perfectly circular shape. No obvious spiral arm structures or prominent dust lanes are discernible. The galaxy exhibits a gradient in its light distribution, with luminosity decreasing smoothly from the central region outward. There are no obvious signs of a major merger event, although the galaxy appears to be interacting with satellite galaxies, based on slight asymmetries in the halo. The colors appear yellow, suggesting the presence of an older stellar population, with the possibility of some ongoing star formation.
