The galaxy presents a generally smooth morphology, with a slight elongation suggesting an elliptical or lenticular classification. The central region exhibits a concentrated luminosity profile, hinting at a potential bulge structure. The overall color is predominantly yellowish-white, transitioning to a bluer hue at the edges, implying the existence of younger stellar populations in the outer regions. No distinct spiral arms or bar features are discernible. There is a subtle asymmetry in the light distribution; however, the light appears evenly distributed. This may suggest minor disturbances such as a small tidal interaction.
