The object presents as a relatively elongated, lenticular galaxy, likely a disk galaxy seen at a moderate inclination. It is luminous, showing a central bulge with a high degree of smoothness in its light distribution, suggesting a lack of significant recent star formation within the nuclear region. 

One arm appears to be relatively smooth, while the other is more disturbed. The galaxy exhibits evidence of having an active galactic nucleus. There is a relatively tight winding of the spiral arms. The colour of the galaxy seems to be relatively red, possibly due to it not forming many stars. The general structure appears elongated, showing a possible cigar shape. There is a distinct lack of large-scale disruptions, but there is one adjacent object that appears to be interacting with the galaxy. The light from this system suggests an old galaxy.