The galaxy presents as a somewhat diffuse, luminous object with a centrally concentrated morphology. The light distribution appears relatively smooth, lacking prominent spiral arm structures or strong bar features. The galaxy exhibits a near-spherical, or slightly elliptical shape. There is a subtle color gradient, with a slightly bluer hue towards the center of the galaxy, suggesting the presence of a younger stellar population in the core. There are no obvious signs of major tidal disturbances or ongoing mergers, although subtle asymmetries cannot be ruled out. Based on the observed color and morphology, the galaxy is likely an early-type spiral galaxy, or a galaxy trending towards a more elliptical morphology. The modest luminosity suggests it is of intermediate mass.
