The galaxy presents an elliptical morphology, elongated with a significant degree of flattening. The central region is characterized by a bright, concentrated nucleus exhibiting a yellowish hue, suggesting an older stellar population. The outer regions display a fainter, diffuse glow with reddish tones, potentially indicating a mix of intermediate-age stars and dust. No prominent spiral arms or distinct features are visible; however, there is some irregularity to the outer shape of the galaxy. The overall color gradient suggests a gradual decrease in star formation activity from the center outwards.
