The galaxy presents a generally smooth morphology with a slight elongation, appearing somewhat disk-like but without readily discernible spiral arm structure. The light distribution is centrally concentrated, with the highest intensity in the core region. Colors range from blue in the core to redder hues in the outer regions, suggesting a possible radial gradient in stellar populations or dust content. The galaxy exhibits a moderate luminosity. There is some indication of minor disturbances in the form of slight asymmetries, though no major merging events appear to be in progress.
