The galaxy appears to be a relatively smooth, elliptical system. Its light profile suggests minimal disk-like structure or spiral arms. The concentration of light is centrally peaked with a gradual decrease in brightness outward from the core. The object exhibits a yellowish-red hue, indicative of an older stellar population and potentially a lower rate of ongoing star formation. There is no obvious evidence of tidal features or significant morphological disturbances suggesting an ongoing or recent major merger event. The galaxy appears well-defined and regular in shape, appearing generally round. A slight asymmetry or minor distortion in the outer regions may be present upon close inspection, possibly hinting at a minor interaction. 
