The galaxy presents as a spiral, viewed at an oblique angle, close to edge-on. A prominent central bulge is visible, exhibiting a bright, concentrated luminosity, with a yellowish hue that suggests a population of older stars. The disk component, extending outwards from the bulge, shows some evidence of spiral arms.

The arms appear relatively smooth, not displaying strong knotty or clumpy structures characteristic of intense star formation regions, but there are some blueish colorations, indicating there are some younger stars. The relative smoothness suggests the galaxy is not undergoing a major merging event.

The disk does not appear heavily obscured by dust lanes, indicating a relatively low dust content. Overall, the galaxy exhibits features consistent with a galaxy transitioning to a more quiescent state in its evolution, with declining star formation relative to its mass. The presence of a possible minor merging event cannot be fully ruled out.
