The galaxy presents a relatively smooth and luminous appearance. It displays a somewhat elliptical morphology, appearing more 'in between' rather than distinctly round or elongated. There are no prominent spiral arms or a strong central bar structure visible. The galaxy exhibits a strong blue hue, suggesting the presence of a relatively young stellar population and ongoing star formation activity. While the galaxy doesn't appear to be undergoing a major merger event, the possibility of minor disturbances or interactions cannot be entirely ruled out given some asymmetry. The observed characteristics align with a galaxy that has experienced some degree of evolution, potentially transitioning from a more actively star-forming phase towards a more quiescent state.
