The galaxy presents a spiral morphology, although partially obscured by distance. The arms are prominent and exhibit a relatively open structure, indicative of grand design spiral characteristics. The central bulge appears moderately sized and exhibits a color gradient towards redder wavelengths. The bluer emission traces the spiral arms, suggesting active star formation along these regions. The dust lanes are observed in the spiral arms. No strong bar structure is apparent. There are hints of disturbance with some morphological asymmetry. Based on the color profile, the object is likely relatively massive and is undergoing significant star formation.
