The galaxy presents as a spiral type, exhibiting a prominent, tightly wound spiral arm structure. The arms are well-defined and extend outwards from a bright central bulge. The bulge appears to be significant in size, contributing noticeably to the overall luminosity of the galaxy. A distinct bar structure appears to be present within the bulge, oriented along the major axis. The disk of the galaxy is observed at an oblique angle, but not quite edge on. There are signs of dust lanes within the disk, particularly along the inner edges of the spiral arms. The overall color profile suggests a relatively evolved stellar population, with a redder hue dominating the bulge region.
