The galaxy presents as a spiral type, with a prominent, relatively bright central bulge. The spiral arms are tightly wound and well-defined, exhibiting a flocculent structure. These arms extend from the central region outwards. There appears to be at least three distinct spiral arms. The dust lanes within the spiral arms are not very dark but appear to be well-defined. The overall color suggests a substantial population of young, blue stars within the spiral arms, which is a typical region of ongoing star formation. The central bulge is yellowish-white, indicating an older stellar population. There is no obvious sign of strong interactions or major mergers, although there might be some minor disturbances in the outer regions of the disk. The galaxy is viewed close to face-on.
