The galaxy presents as a spiral type, with prominent spiral arms. These arms emanate from a central bulge region, characterized by a bright, concentrated core. The arms display a fairly tightly wound morphology, tracing a relatively closed pattern around the central bulge. A bar structure appears present. The bulge exhibits moderate size. The central region of the galaxy displays a yellowish-white hue, likely indicating an older stellar population. The arms are slightly bluer. The disk appears relatively thin. The galaxy does not show significant signs of major mergers or tidal disturbances. The spiral arms are well-defined, suggesting a relatively undisturbed structure.
