The galaxy appears as a luminous, centrally concentrated object with a smooth, symmetrical profile. Its morphology is predominantly elliptical, exhibiting a high degree of roundness. There is minimal evidence of spiral arm structure or prominent disk features. The light distribution suggests a centrally dominant bulge component, with a gradual decrease in luminosity outwards. Faint, diffuse extensions are hinted at but do not disrupt the overall smooth appearance. There is no clear sign of recent major merger events.
