The galaxy presents as a moderately luminous object, exhibiting a generally smooth morphology with a central concentration of light. The core appears reddish, suggesting an older stellar population. Surrounding the core is a somewhat elongated, diffuse halo of bluish light, implying the presence of younger stars and possibly ongoing star formation, although at a moderate rate. No distinct spiral arm structures or prominent dust lanes are discernible within the observed image resolution. The galaxy appears relatively undisturbed, with no significant signs of tidal interactions or major mergers. The overall structure suggests a morphology that is somewhere between elliptical and lenticular, showing a gradual transition in color from the center to the outer regions.
