The galaxy appears to be a relatively smooth object, lacking prominent spiral arms or a distinct disk structure. It exhibits an elliptical morphology, elongated in shape. The galaxy's core region shows a concentrated luminosity, suggesting a high density of stars. The color profile indicates a redder hue in the central regions, potentially signifying an older stellar population, whereas the outer edges tend towards bluer shades, potentially signifying younger populations of stars. Overall, it appears undisturbed with no major ongoing mergers, showing only hints of minor perturbations. The light distribution gradually fades away from the core, showing a smooth transition into the background sky.
