The galaxy presents as a disk-shaped structure, exhibiting a relatively smooth morphology with a possible bulge-like central concentration of light. The color profile appears to shift from a bluer hue in the outer regions of the disk to a more yellowish-white tone towards the center. The axial ratio suggests a moderate inclination with respect to the observer. The overall impression is that of a galaxy undergoing relatively quiescent star formation, possibly with a stellar population that is somewhat older in the central regions. The galaxy doesn't show any major disturbances, distortions, or tidal features indicative of recent mergers or strong gravitational interactions. The galaxy appears to be relatively isolated.
