The galaxy presents a generally smooth and concentrated morphology. It appears elliptical in shape, exhibiting a moderate degree of elongation, trending towards a cigar-like appearance. The central region of the galaxy is characterized by a bright, luminous core, indicative of a high concentration of stars. The luminosity gradually decreases moving outward from the center, forming a diffuse halo. There is little evidence of spiral arms or distinct structural features. The galaxy is overall relatively undisturbed, showing minimal signs of interactions or merging events. The color profile indicates a population of relatively old stars. There may be ongoing star formation, but at a low rate.
