The galaxy presents as an elliptical structure with a smooth, largely featureless appearance. The central bulge is dominant, exhibiting a concentrated luminosity that decreases radially outwards. The galaxy displays a slightly elongated shape. There is minimal evidence of spiral arm structures or dust lanes. The color profile indicates a generally older stellar population, with a reddish-yellow hue dominating the central regions. There are subtle color variations in the outer regions, with hints of bluer components, possibly indicating regions of recent, or ongoing star formation, albeit at a low rate. There are no obvious signs of a major merger or significant tidal disturbances.
