This galaxy exhibits a smooth morphology, displaying a largely featureless structure without prominent spiral arms or distinct clumps of star formation visible in this image. The overall shape is elongated, resembling a cigar or elliptical form. There appears to be a radial color gradient, with the central region appearing bluer relative to the outer edges. This suggests a potential concentration of younger, hotter stars towards the core. Though the morphology is largely smooth, there is a slight asymmetry that indicates a potential disturbance or interaction event.