The galaxy presents a predominantly smooth morphology, with a high degree of central concentration. It exhibits an elliptical shape, appearing somewhat elongated. The central region displays a bright, yellowish hue, suggestive of an older stellar population. A faint, blueish disk-like structure can be observed surrounding the central bulge. There are hints of some minor disturbances. The galaxy is not exhibiting an actively merging state with other galaxies. Overall, this galaxy appears to be an intermediate-mass system with a moderate redshift. Star formation appears to be present, but likely at a relatively low rate.
