The galaxy appears as a relatively compact and smooth object with a near-circular morphology. It exhibits a central concentration of light that fades gradually toward the edges, suggesting a lack of distinct spiral arms or a prominent disk structure. The color profile indicates a generally blue hue, with the central region appearing slightly more cyan. The smooth appearance and color suggest that this is likely an elliptical galaxy with some ongoing star formation, but not at a very high rate. There is no evidence of any major merger events or tidal disturbances in this image. The galaxy presents a well-defined, singular structure, indicating that it is likely in a relatively stable state.
