The galaxy presents as a lenticular or possibly spiral galaxy viewed edge-on. The central bulge is prominent and appears smoothly distributed with high luminosity. A faint, diffuse disk extends from the central bulge and appears relatively thin. There is little to no evidence of distinct spiral arm structure or active star formation within the disk. The galaxy exhibits a reddish hue, suggesting an older stellar population is dominant. The overall morphology indicates a relatively evolved system, potentially transitioning to a more quiescent state. There are no apparent signs of tidal disturbances or interactions with nearby galaxies, suggesting it is currently undergoing a period of relative isolation.
