This galaxy presents as a spiral galaxy, with moderately defined spiral arm structures emanating from a central bulge. The arms are grand design and have a high degree of symmetry. The bulge appears relatively small and is concentrated. The galaxy has no evidence of ongoing major merging activity or strong tidal disturbances. Some regions within the spiral arms may have active star formation, showing localized, concentrated areas of bluer light. The overall color profile is mostly a smooth continuum across the optical spectrum. The disk is observed nearly face-on. There may be evidence of a bar structure, although it is not pronounced. The stellar mass is significant, with what seems to be a considerable star formation rate. The galaxy has a smooth appearance, with a few distinct features present.
