The observed galaxy presents a distinct spiral morphology. The galaxy's disk structure is clearly visible, exhibiting well-defined spiral arms. These arms appear tightly wound around the central bulge. The bulge itself is moderately sized, contributing significantly to the overall luminosity of the galaxy. There appears to be two main arms, however, some areas look too dim to properly be determined. The colour of the galaxy suggests on-going star formation activity, particularly within the spiral arms. No obvious bar structure is detected. The galaxy does not display any significant signs of tidal disruption or major merging activity. There might be a minor disturbance in the morphology, possibly hinting at a past or ongoing minor interaction.
