The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth morphology with no immediately discernible spiral arm structure. Its shape is moderately elongated, possessing a high degree of central concentration. The color gradient suggests an aging stellar population, with a yellowish-red hue dominating. There is very little evidence of ongoing star formation. Subtle indications of disturbance could imply a minor past or ongoing interaction, though a major merger seems unlikely.
