The galaxy appears as a centrally concentrated, generally smooth structure with a roughly elliptical morphology. The light distribution suggests a relatively evolved system, with a dominant spheroidal component. Color gradients are subtle, possibly indicating a relatively homogeneous stellar population across the galaxy's extent. Faint disk-like features may be present but are poorly defined. There is no significant evidence of ongoing major mergers or tidal disturbances. The morphology is most consistent with an early-type galaxy, such as an elliptical or lenticular galaxy. The light is relatively uniform and centralized, indicating older stellar populations are dominant.
