The galaxy presents a roughly cigar-shaped morphology, indicating an elliptical form. The central region exhibits a concentrated luminosity, appearing smooth and yellowish-white, possibly indicative of an older stellar population. Fainter, reddish hues are observed on the periphery of the galaxy, particularly at the extreme ends of its elongated shape. There is a slight asymmetry in the spatial distribution of light with one edge of the galaxy being more sharply defined than the other, possibly due to dust. The galaxy is an isolated system, with no apparent signs of a major merger.
