The galaxy presents a distinct disk-like morphology, viewed nearly edge-on from our line of sight. The dust lane is prominent, obscuring a significant portion of the galactic plane and contributing to its reddish color. There is a slight asymmetry, potentially indicative of past or ongoing interactions. The galaxy exhibits a relatively smooth appearance, with minimal evidence of prominent spiral arms or intense star-forming regions. This galaxy shows a mass around 10^11.5 solar masses and is not very active in star formation.
