The galaxy presents as a slightly elongated, diffuse object. It appears to have a central bulge that is brighter and more concentrated than its outer regions. There is a hint of a disk-like structure extending from the bulge, but it is not well-defined. The color profile suggests a population of both older, redder stars and younger, bluer stars are present. There is a slight asymmetry visible, hinting at possible minor gravitational interaction or internal disturbances. Overall, it appears to be a galaxy undergoing some form of evolution or interaction.
