This galaxy presents as a spiral galaxy with a moderately inclined disk relative to our line of sight. The central bulge appears prominent and exhibits a yellowish hue, suggesting a population of older stars. The spiral arms are well-defined, exhibiting a tightly wound structure. Blue regions are observed within the arms, indicative of active star formation. These areas likely contain younger, hotter stars. There is a faint indication of a bar-like structure crossing the central bulge. No obvious signs of major interaction or merging are visible.
