The galaxy presents as a slightly inclined disk galaxy, potentially a spiral. The central bulge appears moderate in size and exhibits a yellowish hue, suggesting an older stellar population. Fainter, bluer regions surround the bulge, likely indicating areas of active star formation within spiral arms. These arms are somewhat fragmented and not sharply defined, giving the galaxy a slightly flocculent appearance. There's evidence of possible tidal disturbances or interactions. Overall the galaxy exhibits features indicating ongoing processes of star formation and interaction. The overall color suggests a mix of stellar populations, with an aging core and active star-forming regions.
