The galaxy presents as a slightly inclined disk galaxy with a prominent central bulge. The bulge appears relatively smooth and concentrated, exhibiting a brighter, more uniform luminosity profile compared to the rest of the galaxy. The disk component shows a subtle blue hue, suggesting ongoing star formation, though distinct spiral arm structures are not clearly resolved at this image resolution. The overall shape appears moderately elongated, hinting at a disk-like morphology rather than a purely elliptical one. There are some indications of minor disturbances or irregularities in the outer regions of the disk, suggesting possible interactions or recent merger events. The galaxy is neither strongly red nor particularly blue, indicating an intermediate stellar population with a moderate rate of star formation.
