The galaxy presents as a relatively compact, centrally concentrated object. Its morphology appears smooth, lacking prominent spiral arms or a distinct disk structure. The galaxy exhibits an intermediate ellipticity, appearing neither perfectly spherical nor highly elongated. A slight asymmetry is observed, hinting at possible interactions or minor disturbances, though no major merger events are immediately apparent. The galaxy's color profile suggests a population dominated by older stars, with a lack of intense blue regions indicative of active star formation. Overall, the galaxy appears to be an evolved system with relatively quiescent star formation activity.
