The galaxy appears as a centrally concentrated, relatively smooth object with a moderate degree of roundness. The light profile suggests a dominant spheroidal component, though there is some indication of an underlying disk. The galaxy exhibits a color gradient, with the central region appearing more yellow/orange, suggesting an older stellar population. Fainter bluish hues are detected in what appears to be the outer reaches of the disk component. There are no apparent signs of significant ongoing mergers or major disturbances, however, there appears to be a slight disturbance or asymmetry in the overall structure. Given the overall morphology and colour profile, it is likely an early-type spiral galaxy.
