The galaxy presents as a centrally concentrated object, exhibiting a generally smooth morphology. There is minimal apparent structure, such as spiral arms or distinct features. The object appears largely spheroidal, with a high degree of roundness. There is no obvious presence of a prominent disk component or ongoing major merging activity. Minor disturbances cannot be ruled out, but the overall structure suggests a relatively relaxed system. The light distribution is dominated by a bright central bulge, potentially indicative of an older stellar population. Based on its color, it likely has modest ongoing star formation.
