The galaxy presents an overall smooth morphology, with a dominant spheroidal component. Its light distribution suggests a centrally concentrated structure. The galaxy appears slightly elongated rather than perfectly circular. While the primary structure seems undisturbed, there is a faint hint of a possible minor interaction or disturbance in the outer regions, although this is not definitive. There appears to be a secondary object in proximity, but it does not suggest a major interaction. The overall color suggests a mix of stellar populations, with an older population dominating the central region and potentially younger, bluer stars in the outskirts. The galaxy shows a moderate level of star formation activity.
