The galaxy presents as a relatively compact and luminous object. Its light is predominantly bluish-white, with a brighter, more intensely blue core. This suggests a significant population of young, hot stars indicative of ongoing star formation. The shape of the galaxy appears elliptical, exhibiting a smooth profile, although subtle irregularities suggest potential minor disturbances or interactions. There is a distinct lack of defined spiral arms or a prominent disk structure. Based on the overall morphology, it likely has substantial mass and moderate star formation activity.
