The galaxy appears to be a lenticular or early-type spiral, exhibiting a predominantly smooth and rounded morphology. A bright central bulge dominates the light profile, surrounded by a fainter, more diffuse disk. The disk component seems to be inclined with respect to our line of sight. Hints of arm structures are possibly present within this disk, but are not well defined. The overall color is yellowish-orange. There may be evidence of a recent merger event or tidal interaction given the somewhat disturbed nature of the outer regions. Based on its color and morphology, star formation rate is likely very low within the galaxy. 
