The galaxy presents a largely smooth, elliptical morphology. Its color profile suggests a population dominated by older stars, exhibiting a yellowish-orange hue. No distinct spiral arms or bar features are discernible. The overall shape appears to be nearly circular. There is no evidence of significant ongoing star formation. There's no major merger or tidal disturbance currently affecting the galaxy's structure, though a minor disturbance cannot be ruled out. The object is relatively compact, with an estimated effective radius of approximately 7 kiloparsecs.