The galaxy appears relatively compact, exhibiting a slightly elongated morphology. It has a central, bright core region. Faint extensions are visible, suggesting a possible tidal interaction or disruption of the galaxy’s structure. There's a secondary concentration of light slightly below the central core, indicating a potential merger event or an area of concentrated star formation. The overall smoothness suggests it might be an elliptical galaxy, but the slight irregularities may indicate otherwise. Based on light detected, the galaxy shows emission in the g and r bands, with significantly lower emission or absence in the z band. This suggests it could be at a moderate distance. More detailed spectral analysis would be beneficial to investigate its composition, redshift, and any ongoing star formation activity.
