The galaxy presents as an elliptical morphology, exhibiting a smooth, featureless light distribution. The core region demonstrates a concentrated brightness, transitioning outward to a more diffuse halo. The overall color profile indicates a redder hue, suggesting an older stellar population and a relatively low rate of star formation. The shape appears elongated, approaching a cigar-like appearance. There is no visual evidence of ongoing major merger activity or significant tidal disturbances. Minor disturbances may be present, but hard to tell given the resolution of the image.
