The galaxy presents as a fairly smooth, elliptical object with a high degree of central concentration. The light distribution appears symmetrical, lacking any obvious spiral arms or bar structures. The color profile suggests a population of older stars, with a slightly redder hue in the central bulge that fades towards the edges. No significant dust lanes or signs of active star formation are apparent. The object's overall morphology indicates it is likely an early-type galaxy, potentially an elliptical or lenticular galaxy, with minimal ongoing mergers or tidal interactions. The relative roundness of the structure suggests that any recent interactions have not significantly disturbed the overall shape of the galaxy.
