The galaxy presents as an elongated, somewhat elliptical structure with a concentrated central bulge. The light distribution is relatively smooth, appearing more diffuse towards the outer regions. The color profile suggests a higher concentration of older stellar populations, indicated by the slightly redder hue in the outer edges, with bluer stars toward the center. The galaxy exhibits a degree of flattening, though lacking prominent spiral arm structures. There is no obvious active galactic nucleus activity visible in the image, but rather a quiescent elliptical morphology.

