The galaxy presents as a moderately inclined spiral, exhibiting a central bulge that appears bright and yellowish-white in color, suggestive of an older stellar population. The disk component surrounding the bulge shows indications of spiral arm structures, though the resolution limits precise definition. These arms display bluer hues, indicating the presence of younger, hotter stars and regions of active star formation. Dust lanes may be present, though obscuration makes them difficult to fully resolve. The overall morphology suggests a disk galaxy with an intermediate bulge-to-disk ratio, and an estimated angular size of roughly 10 arcseconds. The galaxy's redshift, at approximately 0.06, suggests a relatively nearby object. The ellipticity of the galaxy indicates a disk seen at an angle, without being edge-on, so spiral structures can still be made out. The color gradients suggest ongoing star formation.
