The galaxy presents as a lenticular or early-type spiral system, viewed at a near edge-on angle. Its morphology is characterized by a prominent, smooth bulge that dominates the central region. This bulge exhibits a concentrated brightness profile. Extending outwards from the bulge is a relatively faint disk. Some dust features are visible in the disk, obscuring portions of the starlight and giving it a mottled appearance. Overall, the galaxy displays a bluish hue, with the central bulge appearing slightly more yellow. There appears to be no evidence of a bright central active galactic nucleus or significant star formation, suggesting a more quiescent or aging stellar population. The lack of obvious spiral arm structure supports a classification towards the earlier types. The galaxy's overall shape is somewhat elongated, lacking a perfectly circular appearance. There are no obvious signs of recent major merger activity, although a slight asymmetry cannot be ruled out.
