The galaxy presents as a spiral type, with notable features indicating active star formation regions. Two distinct spiral arms are visible, exhibiting a medium winding pattern, indicative of differential rotation. One arm is particularly well-defined, displaying bluer hues suggesting a greater concentration of younger, hotter stars. The disk component appears prominent, with a relatively low inclination angle from our line of sight. A bar structure seems to be present within the central bulge, although not overwhelmingly strong. The bulge itself is moderate in size compared to the overall disk. There is a possible minor interaction happening with a companion galaxy close by. The overall color suggests that the galaxy is middle aged and not the most luminous galaxy, but still a decent size. 