The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a noticeable spheroidal morphology. There is a lack of prominent spiral arms or a well-defined disk structure discernible in the image. The galaxy appears nearly round in shape. There is a slight color gradient, with a brighter, whiter core and a gradual shift towards a slightly redder hue in the outer regions. There is no evidence of ongoing mergers or tidal disturbances. The light distribution suggests a relatively evolved system, potentially an elliptical galaxy or a lenticular galaxy with a significant bulge component. Star formation appears to be relatively quiescent within the galaxy.
