This galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth, featureless morphology. The light distribution appears centrally concentrated, with a high degree of roundness and minimal indication of spiral arms or a prominent disk structure. Its color profile suggests an older stellar population with a significant component of evolved, redder stars, but it also displays some bluer wavelengths indicating star formation. Evidence suggests possible minor gravitational disturbances or tidal interactions. The shape of the galaxy is close to round, with a slightly elongated structure.
