The galaxy exhibits a prominent spiral structure. The spiral arms are well-defined, with considerable dust lanes visible within the arms. The galaxy's bulge is moderately sized, with an elliptical shape that transitions smoothly into the disk. Star formation appears present throughout the galaxy, with regions of bluer light indicating active star-forming regions, particularly along the spiral arms. The galaxy disk shows some signs of disturbance or tidal interactions. A faint, elongated structure extends outwards from the main disk of the galaxy, hinting at a possible tidal tail or the remnants of a minor merger event. The galaxy's overall color suggests a mix of stellar populations, with a considerable fraction of older stars within the bulge and more recent star formation activity evident in the spiral arms. The galaxy shows no clear evidence of a strong bar feature.
