The galaxy presents as an elliptical morphology, elongated with an approximate axis ratio of 3:1. Its light profile appears centrally concentrated and relatively smooth, lacking prominent spiral arm structures or distinct star-forming regions. The dominant color is a yellowish-red hue, suggesting a relatively old stellar population with a paucity of young, massive stars. There is a bluer object located adjacent to the galaxy, indicating a potential tidal interaction or close companionship. There is no obvious evidence of a major ongoing merger or significant tidal disruption.
