The galaxy presents a smooth, elongated morphology. It appears as a flattened, cigar-shaped structure, lacking any immediately discernible spiral arms or distinct features. The light distribution is concentrated towards the center, exhibiting a gradual decrease in intensity towards the outer edges. The color profile suggests a redder population of stars, with a subtle blue hue present at the ends. There appears to be little evidence of recent major merger activity or significant tidal disturbance. Overall, the galaxy resembles an elliptical galaxy with a relatively high degree of smoothness.
