The galaxy presents as a moderately faint, elongated structure. Its central region displays a relatively smooth appearance with a gradual increase in luminosity toward the core. The overall color is indicative of a population of older stars. There is faint evidence of a possible disk-like structure, though it's not sharply defined. There may be slight disturbances in the morphology, indicating a minor gravitational interaction in the past, though a major merger seems unlikely based on the overall structure. The lack of bright, blue regions suggests relatively low current star formation activity within the galaxy. Its apparent shape suggests that this galaxy has a low inclination angle relative to our line of sight.
