The galaxy presents a morphology consistent with an elliptical galaxy. It exhibits a smooth, diffuse light distribution, with a high degree of central concentration. The color profile suggests a population dominated by older stars, displaying a reddish hue. There is no discernible evidence of spiral arms, a distinct disk, or active star formation regions. The galaxy appears generally undisturbed, with no obvious signs of tidal interactions or mergers. A slight elongation is observed, indicative of a deviation from perfect sphericity.
