The galaxy presents as a single, moderately bright object with a roughly elliptical morphology. There is a dominant central concentration of light, appearing smooth and somewhat rounded. Evident is a notable color gradient, shifting from yellower hues at the core to bluer tones in the outer regions of the galaxy. The central region exhibits a smooth, relatively featureless texture, suggesting a population of older stars. Moving outwards, a faint, diffuse halo is observed, displaying a subtle clumpy structure that indicates some star formation activity within the galaxy. There is evidence of a possible ongoing or recent merger event or tidal interaction, with some irregularity in the galaxy's outer regions. The overall appearance suggests a galaxy that is somewhere between an elliptical and a spiral galaxy that is currently merging with another galaxy.
