The galaxy presents a largely smooth, elliptical morphology. The central bulge appears concentrated and exhibits a yellowish-gold hue, suggestive of an older stellar population. There is little evidence of distinct spiral arms or active star-forming regions within the visible spectrum. The galaxy appears relatively isolated with no obvious signs of ongoing major mergers or significant tidal disturbances. Its overall shape is near-spherical, exhibiting a high degree of roundness. The color gradient suggests a generally uniform stellar population with potentially some slight variation in metallicity and age distribution from the core to the outer regions. The galaxy has a diameter of approximately 4 kiloparsecs, making it a moderately sized galaxy. Given the older stellar population and lack of active star formation, this galaxy may be classified as a quiescent elliptical galaxy at a redshift of approximately 0.21.
