The galaxy presents as an edge-on spiral, exhibiting a prominent dust lane bisecting the galaxy along its major axis. The central bulge appears relatively large and has a rounded morphology. The disk component is clearly visible, although without detailed resolution of spiral arm structure due to its edge-on orientation. Color gradients are apparent, with a yellower hue dominating the central bulge, possibly indicative of an older stellar population. Fainter, bluer regions are observed within the disk, potentially tracing areas of active star formation. There's no obvious sign of major mergers or strong tidal disturbances within the visible structure of the galaxy. The overall luminosity suggests a galaxy of significant mass, and a moderate rate of star formation is plausibly present.
