The galaxy presents as a lenticular structure. It exhibits a generally smooth appearance with no immediately discernible spiral arm structures. The object appears elongated, with an axial ratio suggestive of an edge-on or nearly edge-on orientation relative to our line of sight. Color gradients suggest older stellar populations are dominant, as indicated by the redder hues concentrated towards the central regions of the galaxy. There is evidence of bluer colors towards the outer disk, possibly indicating ongoing, though subdued, star formation in these regions. There are no obvious signs of strong tidal interactions or mergers with other galaxies. The object's morphology is largely undisturbed, without any prominent distortions or asymmetries in its overall shape.
