The galaxy presents a generally smooth, elliptical morphology, exhibiting a concentrated central bulge. The overall color profile suggests a dominance of older stellar populations, indicating relatively low current star formation activity. A faint disk-like structure, oriented roughly horizontally, is potentially visible, characterized by subtle color variations which could indicate the presence of small pockets of younger stars or dust lanes within the disk. Overall, the galaxy shows possible evidence of past or ongoing interactions, given the subtle disturbances in its outer regions. There might be an ongoing merger contributing to the overall shape and structure of the galaxy.
