The galaxy presents a largely smooth and rounded morphology, with minimal discernible features suggestive of spiral arms or a prominent disk. Its color profile indicates a concentration of older stellar populations, trending toward the redder end of the spectrum. There is a concentrated central bulge of old stars. The absence of significant dust lanes or irregular structures implies it is a relatively evolved system, potentially an elliptical or lenticular galaxy. The galaxy appears undisturbed, showing no apparent signs of recent or ongoing major merger activity. Overall, the galaxy appears as a well-established, quiescent system.
