The galaxy presents as a single, moderately luminous object with an apparent smooth morphology. The dominant color is yellowish-orange, suggesting an older stellar population. The light profile appears relatively concentrated, with no distinct spiral arms or bar features discernable. The general roundness indicates minimal rotational flattening or tidal distortion. There is some asymmetry, which appears to be the merging of a second, smaller object within the larger. This merging does not create any extreme disturbances to the galaxy.