The galaxy presents as a spiral type, observed at a near face-on orientation. There is clear evidence of spiral arm structure emanating from a central bulge region. The spiral arms exhibit a flocculent morphology, appearing somewhat patchy rather than continuous. The bulge appears moderately sized, with a concentrated brightness profile, suggesting an older stellar population. The arms display a range of colors with possible faint blue regions suggestive of ongoing star formation and redder regions representing older stellar populations and dust lanes. The overall color index indicates a galaxy that is relatively red, indicative of either a higher redshift, an older stellar population, or significant dust obscuration. No obvious signs of tidal disturbances or a major merger are apparent, although subtle asymmetries could indicate minor interactions. The overall structure appears relatively undisturbed with a disk component that dominates the light output.
