The galaxy presents as a relatively smooth, single structure. Its overall morphology is elliptical in shape, appearing neither highly flattened nor particularly elongated. The color profile indicates a bias towards redder wavelengths, suggesting a stellar population dominated by older, less massive stars, and a relatively low rate of ongoing star formation. There is no apparent dust lane obscuring the galactic nucleus, nor any evidence of spiral arm structure. It appears to be a gravitationally relaxed system, undisturbed by recent major merger events. There is no visual sign of any tidal tails or asymmetries, hinting at any ongoing or recent galaxy interactions.
