The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a spheroidal morphology, appearing largely featureless with no readily discernible spiral arms or prominent dust lanes. The light distribution suggests a relatively even stellar population. There are no indications of significant tidal disturbances or ongoing major mergers. The galaxy appears somewhat round in shape with no apparent elongation or asymmetry. There is a slight color gradient, with the core appearing to be a lighter yellow and becoming slightly redder towards the outer edges.
