This galaxy exhibits a somewhat amorphous structure, lacking a well-defined spiral arm morphology. The central bulge appears prominent and exhibits a yellowish-white color, suggesting an older stellar population. Surrounding the central bulge is a fainter, more diffuse disk component, with a slightly bluish tint that indicates the presence of some younger stars. There is some evidence of minor disturbances in the outer regions of the galaxy, possibly hinting at past or ongoing interactions. The overall light distribution suggests a significant population of stars, possibly around 10^10 solar masses, and a moderate rate of star formation is apparent.
