The galaxy presents as a relatively smooth, concentrated object. The light profile appears centrally concentrated with a high degree of symmetry, indicating a likely early-type morphology, perhaps an elliptical or S0 lenticular galaxy. The core exhibits a bright, intense luminosity, fading gradually into the outer regions. There is little evidence of spiral arm structure or prominent dust lanes. The overall shape leans towards circular, though a slight elongation might be present. No major merging or strong tidal disturbances are visibly apparent. It appears to be a rather undisturbed, quiescent system. The color suggests an older stellar population.
