The galaxy appears as a centrally concentrated object with a generally smooth morphology. It exhibits a somewhat elliptical shape but is generally round. The central region is dominated by a yellowish-orange hue, suggesting an older stellar population. Fainter, diffuse extensions of bluish color are observed around the brighter core, indicative of younger stars and potential star formation regions. There is some evidence of minor disturbance in the galaxy's structure, possibly due to a past interaction or merger event, with some asymmetry visible in the outer regions. Overall, the galaxy presents as an evolved system, likely a massive galaxy with a relatively low star formation rate.
