The galaxy appears to be a spiral galaxy, presenting with a moderate inclination relative to our line of sight. Two prominent spiral arms emanate from a central bulge region. The arms are relatively tightly wound and continuous, exhibiting a mottled texture indicative of active star formation regions or dust lanes. The central bulge is luminous and elongated, possibly suggesting the presence of a bar structure. The overall color of the galaxy is slightly redder than the spiral arms, which may indicate an older stellar population or higher dust content in the bulge region. There are no obvious signs of a recent or ongoing major merger, though minor disturbances are possible given the overall morphology.
