The galaxy presents as a slightly elliptical, disk-like structure with a prominent bulge. The central region exhibits a yellowish hue, indicating an older stellar population and lower rates of star formation. A fainter, bluer disk surrounds the central bulge, suggesting the presence of younger stars and ongoing star formation. The galaxy's overall morphology appears relatively undisturbed with no major mergers or interactions evident, although there may be some minor disturbances visible. The galaxy appears to be viewed at a moderate inclination angle, allowing a partial view of the disk structure. The galaxy measures approximately 6.5 kpc across its half-light radius.
