This galaxy exhibits a distinct spiral structure, characterized by two prominent arms. The winding of the arms is of an intermediate nature, neither tightly wound nor loosely extended. A moderate bulge is visible at the galactic center, contributing to the overall luminosity profile. The galaxy displays features suggesting the possibility of minor disturbances or interactions, although a major merger event is not immediately apparent. The disk is viewed at an angle, allowing for a clear observation of the spiral arm structure. While the presence of a bar feature is suspected, its classification remains ambiguous, leaning towards either a weak or nonexistent bar. Color gradients are noticeable, with the central bulge appearing yellowish and the spiral arms exhibiting bluer hues, indicative of ongoing star formation.
