The galaxy presents as a somewhat elongated, elliptical structure. Its color profile suggests an aging stellar population, exhibiting a central bulge with a yellowish hue. Fainter, blue-tinged regions are observed extending from the central bulge, potentially indicative of pockets of more recent star formation within a disk-like component. While largely smooth in appearance, there is a slight asymmetry along the major axis, hinting at a possible minor interaction or past merger event. The galaxy displays a moderate degree of redshift, implying a substantial distance. The overall morphology suggests a galaxy transitioning towards a more quiescent state, possibly evolving from a spiral to a lenticular or elliptical type.
