The galaxy presents as a centrally concentrated spheroid, exhibiting a smooth, relatively featureless morphology. The light profile is centrally peaked, with a gradual decrease in intensity outward. A prominent bulge component is evident, contributing significantly to the overall luminosity. Color gradients are subtle, with a slightly yellower core transitioning to redder hues in the outer regions. The absence of distinct spiral arms or prominent dust lanes suggests a classification toward the early-type end of the Hubble sequence. There is no strong evidence of recent or ongoing major merger activity based on visual inspection, but a slight asymmetry exists.
