The galaxy presents an elliptical morphology, appearing largely smooth and featureless in the image. It exhibits a central concentration of light, indicative of a bulge, which is surrounded by a more diffuse halo. The color gradient suggests the presence of older stellar populations dominating the galaxy's composition. The galaxy appears elongated, displaying a cigar shape. There is no obvious indication of active galactic nuclei activity or recent major merger events within the galaxy. Faint disturbances may be present but difficult to see, and it appears to be a relatively isolated system in its immediate vicinity.
