The galaxy presents as a single, dominant object with a generally elliptical morphology. The light distribution appears smooth and concentrated, with a gradual decline in intensity from the center outwards. The galaxy's core exhibits a yellowish hue, suggesting a population of older stars. Progressing outwards from the core, the color shifts subtly towards a redder tone. There is no discernible spiral structure or any distinct disk component evident in the image. There is no evidence of any major mergers, tidal tails, or strong interactions with any companions. The galaxy exhibits a high degree of central concentration. There is no indication of ongoing or recent significant star formation activity.
