The galaxy presents a generally elliptical morphology, though subtle asymmetries are discernible. A slightly brighter, more concentrated central region is apparent, surrounded by a more diffuse halo. The color profile suggests a mix of stellar populations, with a yellowish hue in the core possibly indicating an older population and a bluer, more extended component suggesting the presence of younger stars. There are some minor disturbances or irregular features in the halo, indicating some previous gravitational interaction with other nearby objects. The galaxy appears to be a disk galaxy.
