The galaxy presents as a spiral type, oriented at an oblique angle to our line of sight. The central bulge appears prominent, exhibiting a concentrated luminosity gradient. The surrounding disk reveals a discernible spiral structure, albeit somewhat flocculent in appearance with a moderate bulge. Two distinct spiral arms can be identified emanating from the central region, tracing outwards.  The overall color profile suggests a mix of stellar populations, with bluer hues in the outer disk regions indicative of ongoing star formation, and redder tones in the bulge region suggesting older, more evolved stars. No significant signs of tidal disruption or ongoing major merger activity are visually apparent.
