The galaxy appears as a centrally concentrated, relatively smooth object with a slightly elongated morphology. There may be some internal structure or a faint disk component, but it is not distinctly visible in the image. The galaxy exhibits a color gradient, appearing bluer in the central regions and becoming redder towards the outer edges. This suggests a difference in stellar populations, with younger, hotter stars concentrated towards the core. The overall color is indicative of a galaxy with ongoing, but low, levels of star formation. There is evidence of a minor disturbance in the morphology; the galaxy could be undergoing a minor merger or tidal interaction.
