The galaxy presents a generally smooth, elliptical appearance, indicative of an older stellar population. Its disk is oriented edge-on relative to our line of sight, obscuring any potential spiral arm structures. The central bulge appears prominent and bright, exhibiting a yellowish hue that suggests the presence of evolved, cooler stars. There's little evidence of significant dust lanes or active star formation regions within the visible light spectrum. The overall light distribution seems relatively uniform and symmetric around the bulge. It has a flattened appearance, but seems relatively smooth and lacks complex morphological features. No sign of mergers.