The galaxy presents as an elongated, edge-on disk galaxy with an apparent axis ratio indicating a significant inclination relative to our line of sight. It possesses a prominent central bulge, which appears to be smoothly distributed, indicative of an older stellar population. There is no readily apparent dust lane visible in the image. The disk component exhibits a fainter, more diffuse glow. The galaxy displays a yellow-red hue overall, with a slight color gradient towards the bulge becoming redder, which suggests a generally evolved stellar population and relatively low current star formation. No signs of tidal disturbances or ongoing mergers are detectable in this image.
