The galaxy appears to be a luminous, elliptical system. Its morphology suggests a relatively smooth distribution of stars, with a high concentration of light towards the galactic center, indicating a prominent bulge. The overall shape is elongated, displaying an aspect ratio that is more akin to a flattened spheroid than a perfect sphere. Color gradients indicate possible variations in stellar populations, with a generally yellow-orange hue, suggesting an older stellar population and potentially low star formation rate. There is no evidence of strong spiral arms, significant dust lanes, or ongoing major merger events. Faint bluer edges suggest slight star formation on the outer edges of the galaxy.
