This galaxy presents as a relatively well-defined, disk-shaped structure, viewed at a significant inclination. The central bulge is prominent, appearing yellowish-white, suggesting an older stellar population. Extending from the bulge are fainter, bluer regions hinting at a spiral arm structure. These arms are not clearly delineated, giving the galaxy a somewhat diffuse appearance. There is some evidence of ongoing star formation within the disk, based on the bluer hue of the outer regions. Overall, the galaxy exhibits characteristics of a relatively massive, moderately star-forming spiral galaxy. There are no indications of major ongoing mergers or tidal disturbances.
