The galaxy appears to be a luminous, elongated structure. It exhibits a somewhat smooth morphology, lacking prominent spiral arms or a well-defined disk. The central region is brighter and more concentrated, suggesting a bulge or core. There is a hint of a possible tidal feature or minor disturbance extending from one side of the galaxy. The color profile indicates a population of older stars, particularly in the central bulge, contributing to the yellowish hue, with some indication of more recent star formation in some spots which seem to have a bluer hue. Overall, the galaxy presents a transition-type morphology.
