The galaxy appears to be a late-type spiral, likely a barred spiral galaxy, with a prominent elongated shape. The bulge is not very prominent, suggesting it's a relatively young spiral galaxy. There seems to be active star formation occurring within its spiral arms, as indicated by the slightly bluer color and patchy distribution of light in the arms. The elongated shape of the galaxy could also indicate tidal disturbances or interactions with other galaxies in its vicinity. There might be some minor disturbance in the galaxy's disk, but overall, it seems to have a relatively undisturbed structure. The major axis of the galaxy appears to have a redder hue in comparison to the galactic poles which seem to have a slightly bluer tint, indicative of active star forming regions.
