The galaxy presents an elliptical morphology, appearing as a flattened spheroid. The light distribution suggests a high degree of central concentration, with brightness decreasing gradually towards the outer regions. The galaxy exhibits a smooth texture, lacking any visible spiral arm structures or prominent dust lanes. There is a noticeable color gradient; the central region appears yellowish-red, shifting towards a more greenish-blue hue in the outer regions. The overall color suggests a stellar population dominated by older stars, with a possible presence of younger stars in the outer regions where star formation might be active. There are no obvious signs of tidal interactions or mergers with other galaxies, with the galaxy appearing relatively undisturbed.
