The galaxy presents a generally smooth morphology, with a central bulge that appears spheroidal and dominates the overall light profile. It exhibits a disk component that is observed close to edge-on. The bulge appears yellowish-white in color, suggesting an older stellar population. The disk component shows a bluer hue compared to the bulge, possibly indicating the presence of younger, hotter stars and ongoing star formation. There is some indication of minor disturbances or irregularities in the disk structure, as evidenced by slight asymmetries and subtle distortions in the outer regions. The galaxy is approximately 7 kiloparsecs in radius and has a mass of approximately 10^10 solar masses. The galaxy has a star-formation rate of about 10^0.5 solar masses per year.