The galaxy appears as a centrally concentrated object with a moderate degree of ellipticity. It exhibits a generally smooth morphology with no distinct spiral arm structures visible. The light distribution suggests a dominant bulge component. There's a suggestion of a very faint disk, or extended halo of stars beyond the central bulge region. The color profile indicates a redder central region, possibly indicating an older stellar population, with a slight bluing towards the outer regions. There is some evidence of minor disturbance in the overall shape, possibly indicating interactions or internal dynamics that are less than completely relaxed. There is not an obvious merging event occurring.