The galaxy presents as a lenticular or possibly a spiral galaxy seen at a high inclination. There is a bright, somewhat amorphous central bulge, exhibiting a concentrated luminosity profile. The disk component appears relatively smooth with a diffuse texture. Some slight irregularities or disturbances can be noticed, and the bluer and lighter regions scattered around the disk suggest regions of possible star formation, though at a low rate. One side shows a hint of a reddish tint. The overall morphology suggests a galaxy undergoing possible minor interaction or past merger event, influencing its current shape and star-forming activity.
