The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated morphology. The light distribution suggests a relatively old stellar population, with a yellowish hue dominating the central region. The outer regions show a subtle gradient towards bluer colors, possibly indicating the presence of younger stars, although this is less prominent. The shape appears moderately elongated, with a noticeable deviation from a perfect circle, suggesting a moderate degree of flattening. There are no apparent spiral arm structures or dust lanes visible, further supporting its classification as an elliptical galaxy. No significant tidal features or signs of recent major mergers are detected.