The galaxy presents as a relatively smooth, centrally concentrated system. The light distribution suggests an elliptical morphology, lacking prominent spiral arms or a well-defined disk structure. The central region exhibits a higher surface brightness, indicative of a galactic nucleus. There is a slight color gradient moving outward from the center, transitioning from a redder hue in the core to bluer tones in the outer regions. There does not appear to be any indication of ongoing major merging activity. The overall impression is of a galaxy with a relatively quiescent stellar population in its central regions, with perhaps a bit of active star formation in its outer edges.
