The galaxy presents a somewhat elliptical morphology, although there is some irregularity to its shape, possibly indicating a disk structure. The central region exhibits a high concentration of light, appearing a yellow hue and consistent with an older stellar population. There is a slight blue color variation in the outer regions compared to the core. The galaxy exhibits some minor disturbances, the structure is blurred suggesting there is a very mild ongoing or recent merger, this might be the cause of the slight bluish hue. The structure has an overall smooth appearance, as well.
