The galaxy presents a generally smooth and featureless appearance, indicative of an elliptical morphology or a lenticular galaxy seen at a significant inclination. Its central bulge appears prominent and exhibits a yellowish-orange hue, suggesting a dominant population of older stars. There is a gradual decrease in surface brightness from the core outwards, with a faint, diffuse halo extending into the surrounding space. The galaxy's shape is slightly elongated, deviating from a perfectly circular form. There is no visual evidence of spiral arms, dust lanes, or active star formation regions. Based on its observed characteristics, this galaxy is likely a massive system with a relatively low rate of star formation, and it shows no signs of recent or ongoing merger activity.
