The galaxy appears to be a spiral galaxy, likely seen at a slight inclination. There is a prominent central bulge region, elongated along what appears to be the galaxy's major axis, indicating the presence of a stellar bar structure.

Two distinct spiral arms emanate from the ends of the bar. These arms are moderately tightly wound and extend outwards. The disk component of the galaxy shows a patchy distribution of bluer light, suggestive of ongoing star formation regions.

There are no obvious signs of significant tidal disturbances or ongoing major mergers. The galaxy exhibits a moderately strong barred spiral structure. The blueness in the arms indicates active star formation regions, which might hint at a younger stellar population in those areas. There is little evidence for a dust lane.
