The galaxy presents as a lenticular, cigar-shaped structure, exhibiting a relatively smooth, featureless morphology. Its light distribution suggests a dominant bulge component with a fainter disk. The central region appears brighter and more concentrated with light, hinting at a possible older stellar population. There is a subtle color gradient, transitioning from a yellowish hue in the core to a slightly bluer tone in the outer regions. The outer disk is relatively indistinct, lacking prominent spiral arm structures. The galaxy does not seem to be undergoing any major mergers or exhibiting significant tidal disturbances. The overall appearance suggests a galaxy that may have exhausted much of its gas supply and experienced a decline in star formation activity.
