This galaxy presents as a spiral type, exhibiting a distinct disk structure. The arms appear tightly wound, suggesting a grand design spiral galaxy morphology. There's a notable central bulge that is moderate in size, though not overly dominant. The arms show some clumpy regions likely indicative of active star formation, but they are primarily dominated by older stars. The color profile suggests the presence of both young, blue stars and older, redder stellar populations. Overall it is a relatively undisturbed galaxy, but with a modest star formation rate.
