The galaxy appears as a centrally concentrated, relatively smooth object. The light profile suggests a dominant bulge component, indicated by the bright, spheroidal core. There is a subtle color gradient, transitioning from a yellower core region towards a redder halo or outer disk. The overall morphology appears largely undisturbed, showing no major signs of tidal features or ongoing mergers, though subtle asymmetries could be present but are difficult to resolve. Its shape appears moderately round. Star formation is likely suppressed, suggested by the redder colors, indicative of an older stellar population.
