The galaxy presents as a centrally concentrated object with a relatively smooth light distribution. It exhibits a generally round morphology, although there appears to be some minor asymmetry or subtle irregularity in its outer regions. The light profile appears to be relatively diffuse, with no clearly defined spiral arms or bar structure visible. There is a hint of possible minor disturbance. The color index indicates that the galaxy is of intermediate color and consistent with an actively star-forming galaxy, suggesting recent or ongoing star formation. Overall, the galaxy appears to be a relatively massive object.
