The galaxy presents as a centrally concentrated object, exhibiting a largely smooth morphology. Its overall shape appears close to circular with a slight elongation. There is no clear evidence of spiral arms or a distinct disk structure. Coloration suggests a dominant older stellar population, with a yellowish-red hue prominent. No major distortions or tidal features indicative of recent major merger events are observed. There is a faint suggestion of slight disturbances in the outer envelope.
