The galaxy presents as a generally smooth and elliptical structure, with a high degree of central concentration. The galaxy is elongated in a cigar-like shape. The color profile reveals a dominant yellowish-orange hue in the core region, suggesting an older stellar population. Fainter blue hues are seen at the edges of the galaxy, hinting at a small degree of star formation. No apparent spiral arms or other distinct features are visible. The overall impression is of an evolved galaxy with minimal ongoing star formation, exhibiting a quiescent morphology. There is a very slight possibility of a minor gravitational disturbance.
