The galaxy presents as a spiral galaxy with a prominent, moderately sized bulge. The disk component appears substantial, exhibiting well-defined spiral arms. The arms show a tightly wound structure. Two spiral arms dominate the galaxy. The nucleus emits a strong luminosity, with the overall morphological structure displaying a significant central concentration. There may be a weak bar structure within the galactic center, as evidenced by the slightly elongated shape of the bulge region. The disk appears slightly inclined relative to our line of sight. No signs of merging activity are evident, although there may be a minor disturbance in the outer disk region, possibly indicative of ongoing interactions. The galactic core contains what looks like a strong active galactic nucleus.
