The galaxy presents a predominantly blue hue, indicative of ongoing star formation. It exhibits a well-defined, moderately sized bulge, which transitions into a more diffuse disk structure. Faint spiral arms are visible within this disk, though they lack sharp definition. There may be a weak bar present, extending from the central bulge. The galaxy does not appear to be undergoing any major merging activity. Based on its color and morphology, it is classified as a spiral galaxy with active star formation.
