The galaxy appears to be a relatively smooth, centrally concentrated object, lacking prominent spiral arms or a distinct bar structure. The light distribution suggests an elliptical or lenticular morphology, with a high degree of symmetry. The color profile indicates a general blueness in the central region that fades out to the edges. The absence of significant dust lanes or clumpy star-forming regions further supports the classification as an early-type galaxy with a quiescent star formation history. There is no evidence of any major ongoing merger activity, although a slight asymmetry may indicate a minor interaction in the past. The overall roundness and lack of elongation confirm the morphological classification as an elliptical galaxy.
