The galaxy presents a somewhat elliptical morphology. It exhibits a prominent central bulge, characterized by a concentrated, bright, yellowish-white hue. The outer regions show a diffuse and fainter luminosity, with hints of a disk-like structure. The color gradient suggests a relatively older stellar population within the bulge, while the disk may contain younger stars. There are no clear signs of spiral arms or significant dust lanes. No major mergers or other disturbances are immediately obvious in the image. There appears to be very little active star formation, based on the weak blue light signature. The galaxy exhibits a moderate redshift, suggesting it is relatively distant.
