The galaxy presents an elliptical morphology, though not perfectly circular. The central region exhibits a higher concentration of luminosity, gradually decreasing towards the outer edges. There is a faint indication of a possible disk-like structure, but it does not appear to be a well-defined spiral galaxy. Patches of slightly darker, more diffuse regions are scattered throughout the galaxy, indicating areas of dust or less dense stellar populations. There are faint indications of possible tidal distortions or minor disturbances in the galaxy's outer regions, which could suggest an ongoing or past interaction with another galaxy, though it is unclear from this image alone. The overall color profile suggests a population of older stars, though with potential for more recent star formation activity present.
