The galaxy presents as a lenticular or early-type spiral galaxy, exhibiting a relatively smooth, elliptical morphology. It is observed nearly edge-on, displaying a slightly elongated shape with a high degree of central concentration.

The color gradient suggests an older stellar population, with a prominent, brighter central bulge indicative of a concentration of evolved stars. There is little evidence of ongoing star formation. No distinct spiral arms are visible in the image.

The overall appearance points towards a galaxy that has largely exhausted its gas supply, exhibiting a reduced rate of star formation. Subtle disturbances or asymmetries might hint at past or ongoing minor interactions.
