The galaxy presents an elliptical morphology, with a smooth and diffuse light distribution. It exhibits a yellowish-white hue at the core, indicative of an older stellar population. The galaxy displays an apparent slight flattening, possibly suggesting it is not perfectly spherical. There is a subtle color gradient from the core outwards, transitioning towards a slightly reddish tinge in the outer regions, potentially indicating a decline in younger, bluer stars further from the galactic center. No distinct spiral arms or prominent dust lanes are discernible within the image. The galaxy appears relatively isolated, without signs of major tidal disturbances or ongoing mergers, though there may be minor disturbances. The shape of the galaxy could be described as somewhere between round and cigar shaped, but more toward round.
