The galaxy presents as a disk-shaped system, observed nearly edge-on. A prominent dust lane obscures a portion of the galactic plane, bisecting the structure. The central bulge appears relatively bright and somewhat elongated along the major axis, exhibiting a smooth texture. Light distribution suggests that this galaxy is dominated by older stellar populations, with an apparent lack of intense star formation activity. Faint, diffuse light extends from the central bulge, indicating a relatively low surface brightness. The overall color index suggests a redder hue, characteristic of evolved stellar populations. No significant tidal features or signs of recent mergers are immediately apparent within the current observational constraints.
