The galaxy presents as a smooth, elongated structure with a high degree of central concentration. It appears to be relatively featureless, lacking prominent spiral arms or distinct dust lanes. The color profile indicates a population of older stars with minimal ongoing star formation. There may be some evidence of minor tidal disturbances in the outer regions, although it is difficult to determine the precise nature without further data. The object shows an indication of a merger event in its past. Overall, the galaxy likely represents an elliptical or lenticular type with an approximate size of 4 kpc, located at a redshift around z = 0.058.
