The galaxy presents as an elliptical or lenticular system, exhibiting a predominantly smooth morphology with minimal discernible features such as spiral arms or a prominent disk structure. The object appears elongated in shape, with a cigar-like appearance and relatively even luminosity distribution across its surface. Its color suggests a stellar population that is somewhat evolved, potentially indicating ongoing, but low level, star formation activity, particularly in the central regions, as indicated by bluer hues there. The galaxy does not show significant signs of ongoing merger activity, as it has a singular nucleus with no obvious tidal tails or disturbed morphologies associated with major mergers. The galaxy appears relatively isolated in its environment, showing no signs of close interaction with any companion galaxies in this field. The outer regions of the galaxy show hints of fainter stellar structures, possibly representing an extended halo.
