The observed galaxy presents as a spiral galaxy, viewed at an intermediate angle relative to its disk plane, meaning it is not perfectly face-on nor edge-on. The galaxy exhibits a prominent, moderately sized bulge, which appears yellowish in color, suggesting an older stellar population. Prominent spiral arms extend from the central bulge. These arms display a relatively well-defined structure, with a winding pattern that transitions from tight near the bulge to looser towards the outer regions of the disk. The spiral arms themselves appear bluish, indicative of active star formation and a younger stellar population. The disk of the galaxy does not appear perfectly smooth, with some evidence of substructure. The galaxy does not appear to be strongly barred, and shows no indications of recent or ongoing major mergers, although there may be some signs of minor disturbance to the disk morphology.
