The galaxy presents as a spiral, with a central bulge that appears moderately prominent. The spiral arms are well-defined and exhibit a relatively tightly wound morphology. Two prominent spiral arms are clearly discernible. The central bulge displays a smoother, yellower color profile, potentially indicating a higher concentration of older stellar populations. The spiral arms show a bluer hue, suggestive of active star formation and the presence of younger, hotter stars. There appears to be a subtle presence of a bar-like structure extending across the central region of the galaxy. There is no obvious evidence of any major ongoing merger events.