This galaxy presents as a disk galaxy, viewed nearly edge-on from our vantage point. A prominent, moderately bright central bulge is visible, appearing somewhat elongated along the major axis. The bulge exhibits a smooth, rounded morphology. The disk component is significantly elongated. Some dust lane structures may be present, but this is difficult to ascertain due to image resolution. No significant signs of tidal disturbances or interactions with other galaxies are readily apparent. The object displays a redder hue in the central region and bluer light towards the outer disk, suggesting a relatively modest ongoing star formation rate within the spiral arms, as well as a population of older stars near the center of the galaxy. The overall appearance of the galaxy suggests it is of intermediate mass, and is at a distance that makes detailed morphological study challenging.
