The galaxy presents as a relatively smooth, elliptical morphology. The central bulge appears to be the dominant feature, exhibiting a concentrated, bright, yellowish-white luminosity. Moving outwards, the intensity gradually decreases with a transition to a more reddish hue in the outer regions of the galaxy. There is minimal evidence of spiral arm structures or prominent dust lanes. The overall shape appears to be slightly elongated, tending toward a more oblate spheroid rather than a perfect circle. Indications suggest that the galaxy is quiescent, with a very low star formation rate. There are no obvious signs of major mergers or significant tidal disturbances influencing its structure.
