The galaxy presents as a faint, moderately sized object with no discernible features. It exhibits a fairly smooth morphology. There is little evidence of spiral arms or a prominent disk structure. Its overall light distribution suggests an elliptical or lenticular classification. The galaxy appears to be isolated, showing no signs of ongoing or recent mergers with other galaxies. Its color profile shows a redder hue in the R band and is faint in the Z band, indicating a population of older stars with minimal active star formation.
