The galaxy presents as a luminous, elongated structure. It is a centrally concentrated system, with a smooth appearance, showing little evidence of spiral arms or patchy star formation regions, suggesting it is likely an elliptical or lenticular galaxy. The galaxy's light is dominated by a yellowish hue, indicating a population of older stars. There may be a slight asymmetry or tidal feature extending from one end, possibly suggesting a past interaction or minor disturbance. The galaxy appears relatively isolated within the observed field.
