The galaxy presents as a spiral type, exhibiting a notable central bulge that appears moderate in size. Traces of spiral arm structure are discernible, though not strongly defined. The disk component appears relatively face-on with no signs of the galaxy being edge on. The color profile suggests a mix of stellar populations, with the central region presenting a yellower hue, indicative of older stars. The galaxy does not show any signs of major disturbances or interactions and appears to be relatively isolated.
