The galaxy presents as a lenticular or early-type spiral galaxy, exhibiting a generally smooth morphology with a slight elongation suggestive of a cigar shape. The light profile is relatively smooth, showing a central concentration of light, indicating a bulge component. There is very little evidence of spiral arm structure or prominent dust lanes within the disk, hinting at a well-mixed stellar population. The galaxy appears bluish-white, which could imply the presence of at least some young, hot stars, however, it is more likely a result of redshift. No major mergers or significant tidal disturbances are apparent, though a subtle, minor disturbance cannot be ruled out. Overall, the galaxy seems to be in a relatively quiescent state of evolution.
