The galaxy presents a spiral morphology, although the structure is somewhat blurred, suggesting a degree of distance and/or internal dust obscuration. There is a noticeable central bulge, appearing yellowish, which may indicate an older stellar population concentrated towards the galactic nucleus. Extending outwards from the bulge are faint spiral arms. The arms exhibit a bluer hue, suggestive of ongoing star formation within. There are a few areas of localized brightness in the arms that could represent star-forming regions or clusters. Overall, the galaxy appears to be a relatively massive system, based on the observed luminosity, with a moderately active rate of star formation. There are no obvious signs of a major ongoing merger, though minor disturbances or interactions cannot be ruled out.
