The galaxy exhibits a prominent central bulge with a moderately sized disk. The bulge appears somewhat spheroidal and displays a yellowish-orange hue, suggesting an older stellar population. The disk structure is discernable, exhibiting some asymmetries and hints of spiral arm structure. The arms are not well-defined, appearing somewhat flocculent. There is evidence of significant interaction or disturbance, potentially a merger event, as indicated by the disturbed morphology and faint tidal features. This galaxy is actively forming some stars, but it is not vigorous. The central bulge is the brightest region of the galaxy.
